The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge, characterized by a yellowish-white hue, indicative of an older stellar population. Moving outward from the core, a subtle transition to a bluish halo is observed. This suggests the presence of a younger, bluer stellar population in the outer regions, potentially from recent or ongoing star formation, although limited. There's no clear evidence of spiral arm structures or significant dust lanes, suggesting a more evolved system. The overall morphology points toward an early-type galaxy with a dominant spheroidal component. Faint asymmetry in the outer halo may suggest a past minor merger event.
