The galaxy appears to be an elliptical type, exhibiting a relatively smooth and diffuse light distribution. The light is slightly elongated in shape, but there are no distinct spiral arms or a prominent central bulge. The overall color suggests a population of older stars, contributing to a reddish hue in some regions. Evidence for a possible ongoing or past interaction is noted based on the asymmetrical shape, as well as a tidal disturbance. This may be a minor disturbance, potentially a previous galaxy merger. There is very little dust absorption.