The galaxy presents as a spiral type, exhibiting a discernible disk structure. The central region is characterized by a bright, prominent bulge, suggesting a concentration of older stellar populations. Faint spiral arms extend outwards from the bulge, although their definition is somewhat indistinct. The arms appear slightly flocculent in nature. Dust lanes are subtly visible within the disk, particularly on the near side of the bulge. The overall color suggests ongoing star formation, particularly within the disk, with some blueish tints. The inclination appears to be approaching face-on. There may be some minor disturbances in the morphology, which could suggest an ongoing or recent merger. The galaxy appears relatively isolated, without obvious close companions or tidal distortions.
