The galaxy presents a somewhat elongated, elliptical morphology. It exhibits a relatively smooth and featureless appearance, lacking discernible spiral arms or prominent dust lanes. The light distribution appears centrally concentrated. The color profile suggests a population of older stars with a slightly bluer hue, implying ongoing or recent star formation at a low rate. The estimated size corresponds to a medium sized galaxy. There is a slight distortion to the galaxy shape that could imply there was a minor disturbance due to a merger event, but the light is relatively uniformly distributed.
