The galaxy presents a generally elliptical morphology, appearing elongated with a moderate axial ratio. The central region exhibits a high surface brightness, suggesting a dense concentration of stars. The overall color profile indicates a relatively evolved stellar population, with a redder hue dominating the outer regions. There is a slight asymmetry in the isophotes, potentially indicative of tidal interactions or recent minor mergers. Faint, diffuse emission extends beyond the main body of the galaxy, forming a halo-like structure. There is some evidence of a faint, disk-like structure that is not perfectly aligned with the brighter central region, with a bluer color profile. The image suggests a relatively smooth light distribution within the galaxy, with no prominent spiral arms or distinct features visible.
