This galaxy exhibits a prominent spiral structure. Arms appear somewhat tightly wound, tracing a path from the central region outwards. The nucleus displays a concentrated luminosity, suggesting a significant stellar population. The galaxy is not perfectly edge-on, but not fully face-on either. A substantial portion of the galaxy is organized in the disk. The bulge appears relatively small. There is no obvious visual indication of major interactions or mergers; however, there are some minor asymmetric features in the disk that could suggest some past minor tidal interactions. The spiral arms have a slightly patchy appearance which indicates ongoing star formation. Overall, the galaxy shows a mixed morphology of spiral arms, a relatively small bulge, and a disk containing areas of increased star forming activity. The observed light suggests a composition of both older stellar populations and regions of active star formation.
