The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a yellowish hue in its central region, which likely indicates an older stellar population. This contrasts with the slightly bluer and more diffuse light observed in its outer regions, hinting at some ongoing, although limited, star formation. The overall shape appears more elliptical, with no discernible spiral arm structures or a significant disk component visible. There is no strong evidence of any major ongoing mergers or tidal disturbances in the image, suggesting it is a relatively undisturbed system. A minor disturbance may be present but difficult to ascertain. The galaxy is neither perfectly circular nor elongated, presenting as somewhat between an elliptical and spherical object.
