The galaxy presents as a relatively smooth, elliptical-like structure. A central bulge dominates the morphology, displaying a yellowish hue indicative of an older stellar population. The galaxy exhibits a slight elongation, appearing somewhat cigar-shaped, rather than perfectly spherical. There is some evidence of asymmetry in the outer regions, hinting at possible interactions or minor disturbances. Faint blue regions on the outer edges of the galaxy are suggestive of some ongoing star formation, albeit at a low rate. No distinct spiral arms are visible.
