The galaxy presents as a spiral type, exhibiting a clear disk structure. Prominent spiral arms are visible, wrapping moderately around the central bulge. The galaxy displays a bar feature that appears relatively strong, extending through the central region. The bulge size is moderate, with a somewhat reduced presence relative to the disk. The spiral arms seem to exhibit a medium winding pattern, neither tightly wound nor loosely spread. Two distinct spiral arms can be clearly discerned. There appears to be no significant disruption or signs of major mergers, suggesting a relatively quiescent state, though minor disturbances are not definitively ruled out.
