The galaxy presents as a moderately luminous, elliptical-like structure. The morphology appears largely smooth and rounded, with a slight elongation along one axis. There is a concentration of light towards the central region, suggesting a prominent galactic nucleus. The overall color index indicates a population of older stars, with a generally redder appearance. There is little evidence of distinct spiral arms or significant dust lanes. The light distribution decreases gradually from the center towards the outer edges, lacking sharp boundaries. I do not notice any major disturbances in the galaxy's shape, such as tidal tails or bridges, which would indicate recent or ongoing major merger events. I note hints of some minor disturbances.
