The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There's a noticeable color gradient from the center outwards; the core exhibits a yellow-orange hue, indicative of an older stellar population, while the outer regions appear slightly bluer, suggesting the presence of some younger stars or ongoing star formation, though limited. No distinct spiral arms or bar features are visible. The overall form is somewhat elongated, exhibiting an aspect ratio that leans towards an elliptical shape rather than a perfectly spherical one. There is a faint suggestion of a disk component. There is no evidence of a major merger, though there may be some minor tidal disturbances or interactions.
