The galaxy presents as a disk-shaped system, viewed at a high inclination. The central region exhibits a bright, concentrated bulge, potentially indicative of an older stellar population. The outer regions show a gradual fading in luminosity, with hints of spiral arm structure, though somewhat indistinct. Overall, the galaxy appears to be relatively smooth in texture with an elongated morphology, possibly a transitional type between elliptical and spiral. There is a subtle color gradient from the center outwards, with the central bulge appearing more red, suggesting a higher concentration of older, cooler stars in that region.
