The galaxy presents as a spiral type, with moderately defined spiral arms that appear somewhat loosely wound. There is an indication of a central bulge region, though it is not particularly prominent. The disk component seems to dominate the overall structure. The galaxy displays a blueish hue, suggestive of ongoing or recent star formation activity. There is no strong evidence of significant tidal disturbance or interaction with other galaxies, although a possibility of minor disturbance cannot be ruled out. The galaxy is neither perfectly smooth nor clearly featureless, possessing a moderate level of internal structure.
