This galaxy exhibits a distinct spiral morphology. While not perfectly face-on, its disk-like structure is apparent. The central bulge region appears relatively compact and bright, indicative of a significant stellar population in the core. Spiral arms extend outwards from the bulge, though they appear somewhat flocculent and not as tightly wound. The arms display a mottled texture, likely reflecting the presence of star-forming regions. There may be a bar structure.

The galaxy shows an overall blue color, suggesting ongoing star formation. The arms show evidence of star formation. However, the central bulge appears more yellow in color, which is typical for regions dominated by older stars. There are also indications of possible tidal disruptions, and the galaxy could be in the middle of a merger with another, though there isn't strong evidence to back this statement.
