The object presents as a somewhat amorphous, moderate-sized galaxy. The light distribution suggests a centrally concentrated core with a more diffuse halo. There appears to be a distinct, very bright nucleus. The galaxy exhibits a predominantly smooth morphology with little evidence of spiral arm structure or significant dust lanes. There is a slight indication of a tidal tail or minor disturbance on one side of the galaxy, suggesting a possible past interaction or merger event. The color of the galaxy is primarily greenish, possibly indicating strong emission lines or a higher proportion of younger, hotter stars.
