The galaxy presents as a spiral type. A central bulge is visible, though not particularly prominent. Two spiral arms are clearly observed emanating from the central region, exhibiting a relatively open, loose winding pattern. These arms appear somewhat flocculent, with variations in surface brightness along their length, indicating regions of potentially active star formation. There is evidence of a possible bar structure across the central region, though it is not sharply defined. There appear to be minor disturbances in the disk, perhaps suggestive of tidal interactions or an ongoing merger event. The galaxy's color suggests that this object is a relatively moderate mass spiral galaxy that is undergoing star formation.
