The galaxy presents as an elliptical-like structure, though some irregularity and subtle distortions are visible. The central bulge is bright and exhibits a yellowish-white hue, suggesting a population of older stars. Extending from the central region is a faint, diffuse disk component. There is evidence of a possible ongoing or recent minor merger, as indicated by a slight asymmetry and potential tidal features. The overall color profile suggests moderate star formation, though it appears more quiescent in the central bulge compared to the outer regions. There is a faint, somewhat disturbed arm-like feature extending from the disk, adding to the impression of an ongoing interaction or disturbance.
