The galaxy presents a largely smooth and concentrated morphology, indicative of an elliptical or lenticular type. Its color gradient suggests a dominant population of older stars, potentially indicating a relatively low current star formation rate. There is some indication of a potential merger event in its recent past based on a slightly irregular shape and the presence of a possible tidal tail or smaller companion galaxy in close proximity. The light distribution is centrally concentrated, without any pronounced spiral arm structure or disk features immediately visible in the available data.
