The galaxy presents as an elliptical morphology, characterized by a centrally concentrated spheroid. It exhibits a smooth light distribution, with a gradual decrease in surface brightness moving outward from the core. There appears to be an absence of significant spiral arm structures or prominent dust lanes. The central region shows a yellowish-orange hue, which may indicate an older stellar population. The outer regions transition towards a bluer color, possibly indicating ongoing, though subdued, star formation. Overall, the galaxy appears relatively undisturbed, without any major distortions or signs of recent major mergers. There is a slight asymetry to the outer halo.
