The galaxy appears to be an elliptical galaxy with a smooth, concentrated central bulge that dominates the overall luminosity. The color indices suggest a redder population of stars, indicative of an older stellar population. The galaxy displays a high degree of central symmetry with no distinct spiral arm features visible. There are hints of a very faint, diffuse halo surrounding the central region, but the signal is weak. No significant signs of tidal disturbances or ongoing mergers are observed. The galaxy appears to be relatively isolated and undisturbed. Overall, the galaxy seems to be a massive, quiescent system.
