The galaxy presents as a spiral type, with a pronounced central bulge that appears bright and moderately large. Faint spiral arms extend outwards from the central region, exhibiting a relatively loose winding pattern. Two spiral arms are discernible. The galaxy's disk shows an inclination relative to our line of sight. The galaxy has a bluer hue overall, especially in the disk, which is indicative of active star formation regions. The presence of a bar feature is not easily discernible, but there is an indication of possible minor disturbances in the overall morphology.
