The galaxy appears elliptical and quite smooth, with a concentrated central bulge. Its color suggests a relatively old stellar population, composed of stars that are redder and older. There is a possibility of a minor interaction, and a merging event might be taking place. The galaxy lacks defined spiral arms or significant dust lanes. The morphology overall is consistent with an elliptical galaxy with minimal ongoing star formation, though star formation might be occurring in different regions of the galaxy. The galaxy exhibits an overall yellowish hue.
