The galaxy presents a generally smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that dominates the overall structure. Extending outwards from the core are less defined regions of diffuse light, giving the galaxy a somewhat elongated appearance. There are hints of fainter structures that appear as subtle extensions or asymmetries that could be signs of tidal disturbances. The color profile suggests a population dominated by older stars, with a yellowish hue observed throughout the galaxy's body, though the hints of color variation may suggest minor star formation is present. Overall, it is a high mass, red galaxy that may be merging with another galaxy.
