The galaxy presents as a largely featureless, elliptical morphology. The light profile appears smooth and centrally concentrated, with a gradual decrease in intensity outwards. The central region exhibits a yellowish-white hue, potentially indicating an older stellar population. Fainter, bluer extensions are visible on the periphery of the galaxy, suggesting the presence of regions with more recent or ongoing star formation. There are subtle indications of disturbances in the outer regions, although they do not appear to be the result of a major merger. Overall, the galaxy appears to be a relatively evolved system, with a dominant spheroid component.
