This galaxy presents as a relatively smooth, elliptical-like structure. The light distribution is centrally concentrated, appearing brightest towards the core and gradually diminishing outwards. There is a slight elongation, deviating from a perfectly circular shape, but no significant disk features or spiral arms are discernible. The color appears overall redder, suggesting an older stellar population. This red color is indicative of a lack of substantial current star formation activity. No obvious signs of a major merger event or significant tidal disturbances are apparent in the morphology. The galaxy exhibits a soft glow with a high degree of central concentration and symmetry. The galaxy exhibits a relatively high mass estimate with no significant recent star formation.
