The galaxy presents as a moderately bright, elliptical-like structure with a smooth, concentrated central bulge. The light distribution appears diffuse, with a gradual decrease in intensity moving outwards from the core. There is a slight elongation or asymmetry to the overall shape, although the galaxy appears largely undisturbed. The central region exhibits a yellow-white hue, indicating an older stellar population. The outer regions show a subtle shift towards a bluer color, suggesting the presence of younger stars, or potentially a trace amount of ongoing star formation. There is no evidence of strong spiral arm structure or a prominent disk.
