The galaxy presents a flattened, disk-like morphology with a major axis that is visibly longer than its minor axis, indicating a significant inclination relative to the observer's line of sight. A bright, concentrated central bulge is apparent, which may imply the presence of a supermassive black hole at the galaxy's core. The disk exhibits a discernible color gradient, appearing bluer towards the outer regions and redder near the central bulge. This color difference likely reflects variations in stellar populations, with younger, hotter stars populating the spiral arms and older, cooler stars concentrated in the bulge. Subtle disturbances or asymmetries are noted in the disk, suggesting a possible minor interaction or merger event in its recent history. There is evidence of faint tidal features extending outwards from the main galactic body, further supporting the potential for past or ongoing gravitational interactions with another galaxy or dwarf galaxy. No prominent spiral arm structure is distinctly visible.
