The galaxy exhibits a bright, concentrated central bulge, dominating its overall structure. A faint, diffuse halo surrounds the bright core, making it difficult to precisely delineate the galaxy's edge. The central region displays a bluish-white coloration, suggesting a population of hot, young stars or active star formation. This region is surrounded by a greenish region of ionized gases. Faint extensions, which may be indicative of tidal interactions or merging activity, appear somewhat irregular. The overall morphology lacks a clear spiral arm structure, making it difficult to classify definitively; however, the apparent disturbances and faint halo suggest that it may have had a more defined shape in the past, or may be the result of artifact.
