The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. There is minimal evidence of spiral arm structure or a significant disk component. The light distribution suggests a high degree of radial symmetry, with the majority of the luminosity concentrated in the core. Faint, diffuse emission extends outwards from the core, gradually fading into the background. The galaxy displays a redder color profile, indicative of an older stellar population and suppressed recent star formation. Close inspection reveals subtle color variations within the central region, which could be caused by variations in stellar populations or dust content. There is no clear evidence of ongoing major mergers, although some minor irregularities in the outer isophotes might suggest past interactions or disturbances. The galaxy appears to be isolated within its immediate environment, showing no strong tidal features or interactions with nearby companions within the image.
