This galaxy presents as a spiral type, exhibiting prominent spiral arm structures. The arms are relatively well-defined and exhibit a loosely wound morphology, with numerous bright knots indicative of active star formation regions. The galaxy’s disk appears inclined at a moderate angle relative to our line of sight. A central bulge is discernible, with a moderate size relative to the overall disk. There is no evidence of a strong bar structure bisecting the bulge region. The galaxy appears to be in a relatively quiescent state, showing no obvious signs of a major ongoing merger. We notice a minor disturbance, or asymmetrical distribution of light in the arms, suggesting some kind of gravitational interaction has occurred.
