The galaxy exhibits a clear spiral morphology, presenting well-defined spiral arms. These arms appear tightly wound around a central bulge. The bulge presents an intermediate size relative to the overall disk, appearing neither dominant nor negligible in scale. Star formation appears to be active within the spiral arms, as suggested by their brighter, bluer color, while the bulge has a more yellow hue. A bar structure is present, but does not appear to be particularly dominant. There is evidence of possible interaction or merging event as the galaxy has a disturbed appearance. There is a noticeable tidal tail extending outward from the main galactic body.
