This galaxy appears to be a relatively smooth, elliptical galaxy, with an estimated diameter of 8 kpc. The core is a bright, concentrated yellow color, suggesting a population of older stars. The outer regions exhibit a more diffuse profile with a slight color gradient towards redder hues, also indicative of an aging stellar population. There is no apparent evidence of spiral arms or a pronounced disk. No major mergers or tidal disturbances are visible, although slight asymmetry could suggest minor interaction in the past. Overall, the galaxy exhibits properties consistent with a relaxed, quiescent system.
