The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape approximates an elliptical morphology, with a slight elongation along one axis. The central region exhibits a bright, yellowish core, possibly indicative of an older stellar population. This brighter region is surrounded by a more diffuse halo, characterized by a bluer hue, suggestive of more recent star formation activity. The galaxy appears largely undisturbed, with no obvious signs of ongoing major mergers or tidal interactions, although there may be some minor distortions in the outer regions. Overall, the galaxy appears to be a transitioning galaxy that is moving towards becoming an elliptical galaxy.
