The galaxy presents a concentrated, elliptical morphology, appearing relatively smooth in texture. The luminosity profile exhibits a centrally bright core, indicative of a significant concentration of stars or potentially an active galactic nucleus, with the intensity gradually diminishing outwards. The color appears generally yellow-red, suggesting a population dominated by older stars. A slight elongation is noticeable, although the overall form remains largely spheroidal. No distinct spiral arms or prominent dust lanes are visible. There is a faint, extended halo region. The object appears isolated, showing no obvious signs of tidal interaction or ongoing merger events, though there are other galactic objects in the distance, possibly an indication of a galaxy group. There may be an indication of minor disturbances present but it is difficult to tell from the imagery. Based on its color and morphology, this galaxy is likely an elliptical galaxy undergoing low star formation.
