The galaxy presents as a spiral type, exhibiting a distinct disk structure. Two prominent spiral arms are wound relatively tightly around a central bulge. A strong bar feature is apparent, bisecting the central bulge. The bulge size appears moderate to small relative to the overall disk. The galaxy displays a predominantly smooth appearance in its central region, with a transition to more defined features in the outer disk. There are no strong indications of major mergers or significant tidal disturbances.
