The galaxy presents as a largely smooth, elliptical morphology. The central bulge is prominent and exhibits a concentrated, yellowish-white hue, suggestive of an older stellar population. Moving outward from the bulge, the color transitions to a greenish hue, potentially indicative of ongoing star formation within the galaxy's disk. The disk appears relatively undisturbed, without significant signs of tidal interactions or major mergers. The overall shape leans toward somewhat elliptical. The arms are not distinctly spiral in structure. The galaxy appears relatively isolated, with no obvious nearby companions or signs of a recent major merger event.
