The galaxy appears as a somewhat elliptical structure, presenting a relatively smooth overall morphology. There is a subtle but visible disk-like component. The light distribution is centrally concentrated, with a bright, slightly yellowish core. The outer regions of the galaxy exhibit a bluer hue, suggesting the presence of some younger stellar populations in these areas. A small portion of the galaxy seems slightly disturbed, hinting at a possible minor gravitational interaction or recent accretion event, though a major merger seems unlikely based on the relatively undisturbed appearance.
