The galaxy appears as a centrally concentrated object with a relatively smooth, diffuse morphology. Its central region exhibits high luminosity, transitioning outward to a dimmer, less defined periphery. The color profile suggests a bluer core region, potentially indicative of ongoing star formation or a younger stellar population in the nucleus. There is evidence of some structural asymmetry or faint tidal features, hinting at a possible past interaction or disturbance, although these features are subtle. Overall, it presents as a galaxy with a dominant spheroid component, potentially an elliptical or S0 type galaxy exhibiting some signs of recent or ongoing activity.
