The galaxy presents as a flattened, elliptical form. The central bulge is a prominent yellowish hue, suggesting a high concentration of older stellar populations. The outer regions exhibit a bluer tint, possibly indicating more recent star formation activity. The galaxy appears relatively smooth in structure, lacking distinct spiral arms or other prominent features. The light distribution suggests a gradual decrease in intensity from the core to the outer edges, following a Sersic profile. The galaxy appears to be relatively isolated.
