The galaxy presents as a barred spiral structure, with two prominent spiral arms emanating from a central bar. The bar itself is clearly defined and substantial within the galaxy's morphology. The spiral arms appear grand in design and are moderately wound, displaying a mixture of tightly and loosely wound segments. These arms are populated with what appear to be star-forming regions, indicated by the patchy, somewhat bluer hue within the arms themselves.

The galaxy possesses a distinct bulge component, though it doesn't dominate the overall structure. The bulge is neither overly large nor entirely absent, suggesting a moderate size relative to the disk. There appears to be no major ongoing merger event, although there seems to be some disruption to the disk.

The overall color profile suggests the presence of both older stellar populations, contributing to the yellowish hue, as well as younger, bluer stars within the spiral arms, reflective of recent or ongoing star formation. The galaxy does not appear to be particularly dusty, as there is no indication of significant obscuration. It is a disk dominated galaxy.
