The galaxy presents a generally smooth, elliptical morphology, though with some minor disturbances that suggest a possibility of a past or ongoing interaction. The overall shape appears quite round. A bright central bulge dominates the core region, fading into a more diffuse halo. There is some subtle color variation within the galaxy, with a bluish tint in the outer regions and a more golden or white hue near the core. This suggests younger, hotter stars may be more prevalent in the outer regions, potentially indicative of some ongoing, albeit low-level, star formation. However, the dominant smooth appearance and lack of prominent spiral arms suggest a relatively evolved system, possibly dominated by older stellar populations.
