The galaxy appears to be a relatively smooth, elliptical-like structure, with a concentrated central bulge. The overall color is yellowish, suggesting an older stellar population. There's a very slight elongation, and a lack of spiral arm structure or significant dust lanes are apparent. The galaxy appears to be in a relatively relaxed state with no major signs of ongoing mergers or tidal disturbances. The light profile seems centrally concentrated, which corresponds to a spheroid component. The faint, redder hue surrounding the core might indicate an extended halo composed of older, redder stars.
