The galaxy presents a well-defined disk structure, exhibiting prominent spiral arms. These arms appear somewhat patchy and loosely wound, suggesting ongoing star formation activity. The central bulge region is moderately sized and appears relatively bright, indicating a significant population of older stars. The galaxy's disk appears inclined relative to our line of sight. Dust lanes are visible within the spiral arms, contributing to the mottled appearance and obscuring some of the starlight. The overall color is a blend of blue and red hues, indicative of both young, hot stars in the spiral arms and older, cooler stars in the bulge. There is no obvious evidence of a recent major merger or tidal disruption, but the presence of slight irregularities in the spiral arm structure may point to minor interactions or internal dynamic processes. A possible bar structure bisects the central region.
