The galaxy appears to be an elliptical galaxy. It exhibits a smooth, concentrated light profile, with no discernible spiral arms or significant dust lanes visible. Its overall shape is close to round. The core region is significantly brighter than the surrounding area, suggesting a higher density of stars. The galaxy appears to be relatively isolated, without any major distortions or tidal features indicative of recent or ongoing major mergers. There might be some indications of a minor interaction, but this is difficult to verify. The primary color of the galaxy appears to be yellow/orange, which indicates that it is primarily composed of older stars. The estimated effective radius is approximately 4 kpc.
