The galaxy exhibits a generally elliptical morphology, appearing relatively smooth in structure, with a high degree of symmetry. The light is concentrated centrally, with a brighter core and a fainter, more diffuse halo surrounding it. There is evidence of a slight flattening, deviating from a perfect sphere. The color distribution indicates a redder central region, likely dominated by older stellar populations, with a subtle blueish tint in the outer regions, which may indicate the presence of younger stars or ongoing star formation, albeit at a low rate. There is no apparent evidence of significant spiral arms, bars, or tidal disturbances suggesting recent major merger events. The galaxy appears to be relatively isolated, with no obvious signs of interaction with neighboring galaxies.
