The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated, bright core that gradually fades into a more diffuse halo. The primary coloration is yellowish, suggesting a population of older stars. There appears to be a slight elongation, with the major axis extending approximately three times the length of the minor axis. The outer regions of the galaxy show hints of a faint, blueish tinge, possibly indicating pockets of younger star formation, although this is not a dominant feature. There is no clear evidence of spiral arms or significant dust lanes. Faint disturbances and asymmetries suggest a possible interaction with a smaller companion galaxy or the aftermath of a past merger event. Overall, the galaxy appears to be a massive, relatively evolved system.
