The galaxy presents as a spiral, with a prominent disk structure. It is moderately inclined relative to our line of sight. Two spiral arms are clearly visible, exhibiting a relatively loose winding pattern. The disk shows some irregularity. The central bulge appears to be of moderate size and is not significantly dominant. There is no apparent bar structure. There may be minor disturbances in the disk, possibly indicating a past or ongoing interaction or minor merger event. The galaxy does not appear to be currently undergoing a major merger.
