The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a bright, concentrated core, suggesting a high stellar density. A gradual decrease in luminosity is observed moving outwards from the core, with no distinct spiral arm structure visible. The overall color appears to be a relatively uniform blue-white, indicative of a population of older stars with little to no current star formation, although there may be some ongoing star formation. The galaxy's shape is generally rounded. There is no obvious evidence of a major merger or significant tidal disturbance affecting the galaxy's structure. Faint, diffuse extensions are possible at the edges of the object.
