The galaxy presents as a system with a smooth, centrally concentrated morphology. Its overall shape appears as an ellipse, being more "in between" round and cigar shaped. There is subtle evidence of some form of disturbance, perhaps indicating an interaction or minor merger event. The galaxy's color profile suggests a population of older stars, with a relatively low rate of ongoing star formation. The galaxy itself has a small apparent size, and the overall smoothness suggests that it has undergone some type of "smoothing" process, potentially related to a post-starburst phase. The galaxy appears to be relatively isolated and exhibits subtle features which may be minor disturbances.
