The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. It is generally elliptical in shape, appearing mostly round but perhaps slightly elongated. There is no discernible spiral structure or prominent disk. The light profile suggests a bulge-dominated system, with a gradual decrease in surface brightness moving outward from the center. Minimal disturbances or tidal features are apparent, suggesting relative isolation and a lack of recent major merger activity. The color indices indicate that it is a red galaxy, with a spectral energy distribution peaking toward the redder end of the visible spectrum. This coloration is consistent with an older stellar population, indicating that star formation is suppressed. Overall, the galaxy exhibits characteristics of a mature, passively evolving system.
