The galaxy presents a flattened, elliptical shape with a discernible disk-like structure. A concentration of luminous material is evident in the central region, possibly indicative of a galactic bulge or active galactic nucleus. The object displays a redder hue in its central regions, suggesting a population of older stars or significant dust obscuration. There are hints of asymmetry or tidal features extending from the main body, possibly indicating a past or ongoing interaction or merger event. A small amount of bluer light can be seen at the edges, indicating a small level of star formation.
