The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a morphology consistent with an elliptical galaxy, though some disk-like features may be present. The galaxy's core region is brighter and appears to be more yellow in color, suggesting an older stellar population dominating this area. The outer regions exhibit a bluer hue, which could indicate ongoing star formation. The galaxy appears to be relatively isolated, showing no clear signs of major mergers or significant tidal disturbances. There is a slight asymmetry to the galaxy's shape, possibly indicating a past minor merger event.
