This galaxy presents as a generally smooth, elliptical morphology. It exhibits a centrally concentrated bulge, with light intensity decreasing gradually towards the outer regions. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the central bulge, transitioning towards slightly bluer tones in the outer regions, potentially indicating some ongoing, though limited, star formation in these areas. The galaxy appears relatively undisturbed, showing no significant signs of tidal interactions or major merger events. There is a possible slight asymmetry in the outer regions, but this may be due to image artifacts or subtle underlying structures. Overall, this galaxy appears to be an evolved system with a significant spheroidal component and a relatively quiescent star formation history.
