The galaxy appears as a relatively smooth, elliptical structure. The central region is characterized by a bright, concentrated light, suggesting a high density of stars, and potentially an active galactic nucleus. The light smoothly fades into the surrounding space. The galaxy's shape deviates slightly from a perfect sphere, appearing somewhat elongated. There is no visible evidence of spiral arms or a prominent disk structure. Faint, diffuse light extends outwards, indicating the presence of a stellar halo or tidal features, but this is not definitive. No significant ongoing merging or major disturbances are immediately apparent from its morphology. There is slight variation in the color, suggesting active star formation.
