The galaxy presents a distinct spiral morphology. The spiral arms are tightly wound, exhibiting a flocculent structure. The central bulge appears relatively small compared to the overall disk size. Evidence of a bar structure is present, though not strongly defined. The galaxy shows indications of minor disturbances or possible interaction with another galaxy or object nearby, but no merger is clear. Dust lanes are faintly visible within the spiral arms. The overall color profile suggests a population of both young, blue stars and older, redder stars distributed throughout the disk. The image hints at multiple spiral arms originating from the central region, though definitive arm counts are obscured by the image's resolution and the winding pattern.
