The galaxy presents a morphology consistent with a spiral galaxy, exhibiting a disk-like structure. Faint spiral arms are visible extending from the central region. A weak central bulge is present. The disk appears inclined relative to our line of sight, showing a somewhat flattened appearance. The galaxy exhibits a blue hue, suggestive of recent star formation activity. There are some disturbances in the structure, but does not appear to be in the middle of a major merger event. The galaxy is likely of intermediate mass.
