The galaxy presents as a disk-shaped structure, viewed at a slight angle relative to face-on. The central bulge region exhibits a bright, concentrated luminosity. The overall color profile suggests that the galaxy is likely a spiral. Although there are no distinct spiral arm structures visible within the disk, the bluer hue around the central core and disk is indicative of possible star formation. The outer edges of the disk appear somewhat diffuse, and there's a slight asymmetry, possibly indicating gravitational interactions or recent merger activity. There are no immediately apparent tidal tails or other major disturbances, but closer inspection may reveal subtle distortions. 
