The galaxy presents as a moderately bright, elliptical-like structure. The central region displays a concentrated, yellowish-white hue, suggestive of an older stellar population. Moving outward from the core, the color transitions to a bluer, fainter halo. This extended halo is not uniform, exhibiting some subtle irregularities that could indicate minor tidal disturbances or ongoing interactions. While a disk structure is not readily apparent, the shape of the galaxy is not perfectly spherical, showing a slight elongation. There may be low levels of star formation. Overall, the galaxy appears relatively undisturbed, showing no strong signs of recent major mergers.
