The galaxy exhibits a morphology that suggests an ongoing or recent merger event. The primary body of the galaxy appears relatively smooth and elliptical. There is an extension or secondary component that is visually connected. The overall color is on the redder end. This suggests an older stellar population and/or significant dust content. There may be a region of elevated star formation present, judging from the slightly bluer hue in the outmost part. The system is not perfectly circular, possessing a slight elongation. The size is estimated to be a bit more than 6 kpc radius. Overall, this galaxy appears to be a dynamically active system.
