The galaxy presents as a relatively smooth, centrally concentrated object with no prominent spiral arms or bar structure evident. The morphology appears predominantly elliptical or lenticular. The object has a largely featureless disc with no strong point sources.

The color gradient transitions from a bluer hue near the center to redder tones in the outer regions, potentially indicative of an aging stellar population and declining star formation in the periphery. The central region exhibits a bright, somewhat diffuse core, possibly containing an active galactic nucleus or a dense concentration of stars. There is no strong morphological evidence of recent or ongoing major mergers or tidal interactions with other galaxies. Small disturbances cannot be ruled out.
