The galaxy presents as a relatively smooth, rounded structure, with a concentrated central bulge. There is minimal evidence of significant spiral arm structures or prominent features usually associated with disk galaxies. The light profile appears to fade gradually from the bright core outwards into a diffuse halo, suggesting a relatively old stellar population dominating the overall emission. The color profile suggests an elliptical galaxy with older stars, with minimal signs of recent star formation. Subtle color variations around the main body may indicate minor tidal interactions or the presence of faint, unresolved substructures. Overall, the galaxy appears well-defined, with a classical elliptical morphology.
