The galaxy presents a generally smooth and featureless appearance. It exhibits an elliptical morphology, appearing as a flattened spheroid rather than a distinct spiral or irregular shape. The central bulge appears bright and concentrated, gradually fading into the outer regions. A subtle disk-like structure may be present, but is not definitively discernible.

There are no obvious signs of active merging or major disturbances, although there are potentially slight irregularities in the outer halo which could be the result of minor disturbance. The galaxy exhibits a color gradient, with the central regions appearing slightly redder than the outer regions. This color difference suggests a variation in stellar populations, with older, redder stars more concentrated in the bulge. The overall color is relatively consistent between the G, R, and Z bands.

The galaxy is estimated to be of considerable size, with a physical radius of several kiloparsecs. It exhibits a measurable redshift, indicating a significant distance and recession velocity. The galaxy's estimated mass suggests it is a substantial system with a relatively modest rate of star formation, and a relatively low specific star formation rate.
