The galaxy presents as a relatively smooth, elliptical-like structure. It displays a centrally concentrated luminosity profile, with the brightest region appearing slightly off-center, possibly indicating a non-uniform distribution of stellar populations or a slightly active galactic nucleus. The galaxy exhibits a color gradient, with a central yellowish-white hue that transitions to a reddish-orange periphery. The presence of a few distinct reddish areas embedded in the main body may indicate localized regions of active star formation or dust obscuration. No spiral arm structures or prominent dust lanes are discernible, suggesting that this is likely an older, more evolved system. There seems to be no major disruption of the galaxy body, suggesting it is not undergoing a major merging event.
