This galaxy presents as a centrally concentrated, relatively smooth object with a moderately elliptical shape. The core region exhibits a bright, bluish-white hue, suggesting the presence of a population of relatively young, hot stars. The light intensity decreases gradually outwards from the core, fading into a more diffuse and reddish halo. There is no clear evidence of spiral arm structure or significant dust lanes. The general morphology points towards an elliptical galaxy or a lenticular galaxy, possibly in a relatively quiescent state of star formation. There are no distinct signs of any major ongoing mergers. The overall appearance indicates a system that is not experiencing significant recent interactions or starburst events, though some minor disturbances cannot be ruled out.
