The galaxy presents as a likely early-type system, possibly elliptical or lenticular, with a relatively smooth and concentrated light profile. The overall color suggests a population dominated by older stars, potentially indicating a lack of significant recent star formation. The galaxy exhibits a somewhat elongated shape. There seems to be a smaller object adjacent to the larger galaxy which could be a smaller satellite galaxy. A minor disturbance or an ongoing merger event cannot be ruled out. The main body of the galaxy displays a noticeable color gradient, becoming slightly bluer towards its edges.
