The galaxy appears to be a relatively smooth, elliptical-like structure. It is centrally concentrated with a gradual decline in luminosity outward from the core. There is no discernible disk structure or spiral arms visible. The color profile suggests the presence of an older stellar population, with a yellow-orange hue dominating the central region and a less pronounced but still present yellow-orange color extending to the outer regions. There might be some minor distortions in the outer regions, which could imply minor tidal interactions with another galaxy at some point in its history. The shape is roughly circular, but not perfectly so, with a slight elongation.
