The galaxy presents a largely smooth, elliptical morphology. The central bulge exhibits a concentrated, bright yellow-orange hue, potentially indicative of an older stellar population. The isophotes appear generally regular, with a slight elongation that suggests a transition away from a perfectly spherical shape. There is little visible evidence of spiral arms or significant dust lanes. The galaxy appears relatively isolated, with no immediately apparent signs of tidal interactions or major mergers. A very faint, diffuse halo surrounds the brighter central region, fading into the background sky. Based on the color and smooth structure, the galaxy likely exhibits low current star formation activity.
