The galaxy presents as a luminous, elliptical-like structure with a smooth, centrally concentrated light profile. It appears to be a relatively mature system, with a dominant bulge component characterized by a yellowish-white color indicative of an older stellar population. There is a slight indication of a flattened disk-like structure in the light distribution of the galaxy. The galaxy exhibits a subtle asymmetry, suggesting a possible interaction or past merger event that may be causing minor disturbances in its overall morphology. Based on the apparent color and morphology, it is possible that this galaxy is still forming stars. Overall, the galaxy appears to be relatively isolated and does not show signs of a major ongoing merger.
