The galaxy appears to be a spiral galaxy, viewed at an oblique angle to our line of sight. The spiral arms are readily apparent, displaying a relatively grand design. Two dominant spiral arms are observed emanating from the central region. These arms display a loosely wound structure, appearing somewhat flocculent in nature with varying intensities. The galaxy exhibits a distinct disk component, inferred from the flattened distribution of light. The central bulge is relatively small, contributing moderately to the overall luminosity of the galaxy. Star formation appears to be ongoing within the spiral arms, as evidenced by localized regions of brighter blue light indicating the presence of young, hot stars. There is no obvious bar structure present at the galaxy's center. There is no indication of a major merger event in the morphology, though minor disturbances cannot be ruled out.
