The galaxy presents as a roughly elliptical, disk-like structure viewed at an oblique angle. It exhibits a smooth, centralized luminosity profile, with the brightest region concentrated towards the core. There appears to be a subtle color gradient, with the core showing a somewhat yellowish hue, potentially indicating an older stellar population. Fainter, bluer extensions can be discerned in the outer regions, suggestive of ongoing or recent star formation. The overall appearance indicates a system that is likely a disk galaxy, possibly with a central bulge, where the arms are tightly wound. There is no visible evidence of significant tidal disturbances or ongoing mergers.
