The galaxy appears as a single, relatively smooth object. It exhibits a generally elliptical morphology, presenting as a mostly round shape. The light is concentrated in the center, indicating a central bulge.

There is a color gradient visible. The central regions show a yellowish hue that likely corresponds to an older stellar population. Fainter, diffuse blue light is present in the outer regions, suggesting the presence of younger stars or ongoing star formation, albeit at a low rate.

The galaxy shows no evidence of strong tidal interactions or recent major mergers, although a very subtle asymmetry is visible in the outer isophotes. The overall light profile seems undisturbed, indicating it is likely an isolated system that has evolved relatively quiescently over cosmic time.
