The galaxy presents as a somewhat elliptical structure. The central region exhibits a concentrated, bright core, yellowish in color, suggesting a population of older stars. A distinct bluish component is observed adjacent to the core, potentially indicative of a region of active star formation. The overall light distribution seems smooth with a somewhat disturbed morphology, hinting at a possible past or ongoing minor merger event. There appears to be a faint, diffuse halo surrounding the central structure, though its extent is difficult to discern. A slight elongation of the isophotes is noticeable. The galaxy does not display prominent spiral arm structures.
