The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is no discernible spiral structure or a distinct galactic disk. The central region exhibits a bright, somewhat reddish core, indicative of an older stellar population. This core is surrounded by a diffuse halo of bluer light, which may suggest the presence of some younger stars or ongoing star formation, though it is subtle. The galaxy appears mostly undisturbed, showing no signs of major mergers or tidal interactions. The overall shape is more in between a perfect circle and a cigar shape. There might be some minor disturbance but it is not immediately visible. The color gradient suggests a radial change in stellar population, with older, redder stars dominating the core, and perhaps some younger, bluer stars populating the outer regions.
