The galaxy presents a face-on spiral morphology, displaying prominent, loosely wound spiral arms. These arms exhibit a fragmented structure, suggesting active star formation regions. The central bulge is moderate in size, and a bar structure appears present. There is a slight asymmetry to the spiral arms, potentially indicating a minor gravitational interaction or internal disturbance. The disk appears relatively thin. The galaxy shows a gradual color gradient, with bluer hues in the spiral arms and redder tones towards the bulge, consistent with a mix of stellar populations. There is evidence of a merging event based on the galaxies irregular shape, and asymmetric light distribution.
