The galaxy presents as a relatively smooth, elliptical-like structure. The core region appears to be the brightest, with a gradual decrease in luminosity moving outwards. The color profile suggests a population dominated by older stars, with a yellowish-red hue across the galaxy. There is no obvious presence of spiral arms or dust lanes. The galaxy exhibits a moderate degree of ellipticity, appearing more elongated than perfectly circular. There is no strong evidence of tidal features or other indicators of recent major mergers, although a slight asymmetry on one side might suggest minor interactions or internal dynamics. Based on the integrated light, the galaxy seems to be fairly massive.
