The galaxy presents as a primarily smooth and rounded structure. It exhibits a concentrated central region surrounded by a diffuse halo. Evidence of a spiral arm structure is present, exhibiting a broken appearance rather than continuous and well-defined arms. The morphology of this galaxy suggests it is undergoing interactions or has experienced tidal disturbances in the past, due to the irregular shape and the discontinuous nature of its arms. Some of the regions along the arm display bluer hues, indicating areas of heightened star formation within the structure. The colors are consistent with a population of aging stars with some pockets of active star formation.
