The galaxy presents as a fairly smooth, elliptical morphology. A concentrated central bulge dominates the visual structure, exhibiting a bright, yellowish hue suggestive of an older stellar population. There is a notable lack of discernible spiral arms or prominent dust lanes. The outer regions display a gradual decrease in luminosity, transitioning to a fainter, more diffuse halo. The overall round appearance indicates a near face-on orientation. No signs of major mergers or significant tidal disturbances are apparent, though a slight asymmetry in the outer halo may indicate minor gravitational interaction in the past. The galaxy appears relatively quiescent in terms of star formation, evidenced by the overall lack of blue color.
