The galaxy presents as a relatively smooth, elliptical structure with a noticeable central bulge. The core region exhibits a yellowish hue, possibly indicative of an older stellar population. A subtle disk-like structure, appearing slightly greenish, surrounds the central region, potentially tracing recent or ongoing star formation. The overall shape suggests a system transitioning towards a more spheroidal morphology. There are no readily apparent signs of major mergers or tidal disturbances, however there are signs of a minor disturbance or faint tidal feature in the outer halo of the galaxy. Based on color gradients, star formation activity appears to be higher in the greenish region.