The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core region exhibits a yellowish-white hue, potentially indicative of an older stellar population. Extending outward from the core, the galaxy transitions to a more diffuse, greenish halo. This color gradient might suggest the presence of younger stars or ongoing star formation in the outer regions, although the smoothness suggests limited spiral arm structure. A slight elongation is discernible, imparting a somewhat cigar-shaped appearance to the overall structure. There appears to be some disturbance visible on the left side of the galaxy, possibly caused by minor interaction.
