The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The core region exhibits a pronounced yellowish-orange hue, suggestive of an older stellar population. Moving outwards from the core, the galaxy gradually fades into a less defined halo characterized by a bluer tint, possibly indicating the presence of younger, hotter stars or ongoing star formation, albeit at a relatively low rate. There is a faint, diffuse structure extending from the central region, but without any apparent spiral arms or prominent features. The overall appearance suggests a mature galaxy with a significant bulge component and a relatively quiescent star formation history. There are no indications of major disturbances or interactions with other galaxies in the immediate vicinity.
