The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge that graduates into a diffuse halo. Color gradients are visible; the core displays a yellowish-orange hue, suggesting an older stellar population, while the outer regions present a bluer tint, possibly indicating younger stars or ongoing star formation at a modest rate. There is no clear evidence of a spiral arm structure or significant dust lanes. A slight elongation is detectable, but the overall shape is largely round. No signs of active galactic nuclei, merging features, or major disturbances are immediately apparent, although minor disturbances cannot be ruled out.
