The galaxy presents as an elliptical morphology, with a high degree of central concentration.  The light distribution appears smooth, with a rapid decline in surface brightness moving outward from the core. There is little to no evidence of spiral arm structures or significant dust lanes. The core region exhibits a yellowish-white hue, transitioning to a redder color in the outer regions, possibly indicating an aging stellar population and a lack of ongoing star formation. The galaxy appears generally undisturbed, exhibiting no signs of tidal tails or major morphological distortions indicative of recent mergers. The overall shape is close to circular, with a very slight ellipticity.
