The galaxy presents a generally smooth and elliptical morphology. It exhibits a prominent central bulge, characterized by a yellowish hue, suggestive of an older stellar population. This bulge is centrally concentrated, exhibiting a high degree of symmetry. The galaxy's overall shape is elongated, with a ratio of major to minor axes greater than 2:1. The color gradient transitions from yellow in the core to a faint bluish tint in the outer regions, indicating the presence of younger, bluer stars in the disk. There appears to be little to no visible spiral structure. No significant signs of tidal disturbances or ongoing mergers are evident.
