The galaxy presents a discernible disk-like structure with a noticeable bulge. There is evidence of spiral arm morphology; however, resolution limitations make it difficult to fully characterize the arm structure or determine a precise spiral classification. The color distribution indicates some ongoing star formation, particularly in the disk. Based on the distribution of light in the disk, the galaxy likely possesses a stellar mass on the order of 10^9 solar masses. The bulge region appears relatively smooth, potentially indicating an older stellar population compared to the disk. There may be a weak bar-like feature. Overall, there are no obvious signs of recent major merger activity. However, there is some possibility of a minor interaction or disturbance, perhaps indicating a small companion galaxy.
