The galaxy presents as a spiral type, with a clearly defined disk structure. The spiral arms appear tightly wound and are fairly symmetrical. Two main spiral arms can be readily identified, although the presence of fainter arm segments suggests a more complex structure. The galaxy exhibits a relatively small bulge. There's evidence of a weak central bar. The overall color suggests an actively star-forming galaxy, with a blueish tint apparent within the spiral arms. There are no signs of major mergers or significant tidal disturbances; however, there seems to be a slight asymmetry in the outer disk, hinting at a potential minor interaction or past disturbance. The galaxy appears relatively isolated and undisturbed, residing in a region of the sky with no obvious major companions.
