The galaxy appears to be a spiral type. Two well-defined spiral arms originate from a central bulge, exhibiting a loosely wound morphology. The arms show a clumpy structure suggestive of active star formation regions. A faint bar-like structure seems to bisect the bulge region. The bulge itself is relatively small, and there is an indication of ongoing star formation throughout the disk. There is no indication of strong tidal features or major disturbances, suggesting that the galaxy is relatively isolated and has not undergone a recent major merger. Overall, the galaxy appears to be a relatively normal spiral galaxy with moderate star formation activity.
