The galaxy appears to be a relatively smooth, elliptical or lenticular type. Its color profile suggests a population of older stars, displaying a yellowish-orange hue, indicating minimal ongoing star formation. The galaxy exhibits a centrally concentrated luminosity profile, with a bright core that gradually fades towards the outer edges. There's no visible evidence of spiral arms or prominent dust lanes. The overall shape is close to circular, with no discernible distortions that would suggest a recent major merger event. However, there might be a faint asymmetry in the outer regions.
