This galaxy exhibits a spiral morphology. It appears to be a disk galaxy, viewed at a relatively low inclination angle, not edge on. The spiral arms are clearly defined, showing a symmetrical pattern extending outward from the central bulge. The bulge itself is small and relatively unobtrusive compared to the overall disk structure. There is no apparent central bar feature.

The disk component is characterized by patchy regions of star formation, evident as slightly bluer concentrations along the spiral arms. These areas are likely sites of active star birth. The overall color of the galaxy suggests a mix of stellar populations, with the bulge appearing more yellow/white, indicative of older stars, and the disk showing bluer tones from younger stars.

There is no evidence of major ongoing merger activity or significant tidal distortions. The galaxy seems relatively undisturbed, with a well-defined spiral structure. The star formation rate appears moderate, based on the color and structural features.
