The galaxy presents as a disk-shaped system, viewed at a slight angle that approaches face-on. It exhibits a prominent central bulge, which is comparatively bright and appears yellow-white in color, suggesting a population of older stars. Fainter and more diffuse light extends from the central region, forming the galaxy's disk. There is a possible weak bar-like structure. Although difficult to discern in great detail, hints of spiral arm structures can be inferred from the subtle variations in the disk's surface brightness. The galaxy is surrounded by a faint halo, exhibiting little to no active star formation. Overall, the galaxy displays characteristics consistent with an intermediate-type spiral galaxy, potentially undergoing a quiescent phase in its evolution.
