The galaxy exhibits a generally elliptical morphology, with a relatively smooth and centrally concentrated light distribution. The core region appears bright and slightly yellowish. The outer regions show a bluer hue compared to the core, indicating the presence of a younger stellar population or ongoing star formation, or perhaps differences in metallicity. There is no apparent strong spiral structure or evidence of a recent major merger event disrupting the overall shape of the galaxy, although there is a slight asymmetry in the outer isophotes. The galaxy appears largely isolated, without any obvious signs of tidal interactions or close companions. There might be a faint hint of a very minor disturbance in the outskirts of the galaxy.
