The galaxy presents as a spiral, viewed at an oblique angle relative to its disk. The bulge component appears moderate in size, with a bright central concentration. The spiral arms are distinct, displaying a multi-armed structure, possibly two dominant arms, with fragments of fainter arms branching off. The arm structure seems primarily medium-wound, with some evidence of more tightly wound segments. The overall color profile is generally blue, especially in the outer arms, indicative of ongoing star formation. A weak bar structure may be present through the center of the galaxy, but this feature is hard to determine with certainty. There is some suggestion of minor interaction with other objects due to distortions in the spiral arms.
