This galaxy exhibits a disk-like morphology, viewed at a high inclination angle. The central region appears as a bright, concentrated bulge, with a relatively smooth texture. A distinct ring structure surrounds the bulge, displaying clumpy, blue star formation regions along its circumference. There is evidence of a potential minor disturbance or interaction, visible as a faint tidal feature extending from one side of the disk. This feature is much less pronounced than the main structure. The disk itself shows hints of spiral arm structure, although these are not sharply defined. The overall color profile suggests a mix of stellar populations, with the blue ring indicative of ongoing star formation, and a more reddish hue in the bulge, potentially indicating an older stellar population.
