The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, largely featureless morphology. The light distribution is highly concentrated towards the center, with a gradual decrease in brightness outwards. It appears to be fairly round in shape. There is little indication of spiral arms or significant dust lanes. The color suggests a stellar population dominated by older, redder stars, consistent with a low star formation rate. No signs of an active galactic nucleus are visible based on its morphology. There is no apparent interaction with companion galaxies or any significant tidal disturbance.
