The galaxy presents a largely smooth, elliptical morphology. It appears to be relatively compact, with a central bulge that dominates the visual appearance. The core of the galaxy exhibits a bright, concentrated luminosity, suggesting a high density of stars or potentially an active galactic nucleus. The isophotes of the galaxy are generally regular and undisturbed, indicating a relaxed dynamical state. There is a slight elongation along one axis, but the overall shape is close to circular. Color gradients are subtle, with a yellowish-white hue in the central regions, possibly indicating an older stellar population. There's no clear evidence of spiral arms, dust lanes, or significant ongoing star formation regions within the visible light. Any disturbances present appear minor. 
