This galaxy presents as a primarily smooth, elliptical-like structure. The central region exhibits a bright, concentrated core, potentially indicative of an active galactic nucleus or a dense stellar population. The overall shape is somewhat elongated but generally rounded. There is a subtle color gradient noticeable, shifting from a bluer hue in the outer regions to a redder tone towards the nucleus, possibly suggesting varying stellar populations or dust distribution. There is no apparent evidence of prominent spiral arms or significant dust lanes. The galaxy seems relatively undisturbed, without obvious signs of ongoing major mergers or tidal interactions. Slight asymmetry may indicate minor past interactions.
