The galaxy presents as a spiral type, with a notable disk structure. The spiral arms are prominent, displaying a relatively open or loose winding pattern. Two main spiral arms are clearly discernible. A central bulge is observed, appearing somewhat subdued and not significantly dominant in size relative to the disk. No obvious bar structure is apparent. There is some evidence of possible tidal features or minor disturbances in the disk, suggesting a possible past or ongoing interaction with another galaxy. Star formation appears to be relatively low.
