The galaxy presents as a moderately bright, face-on spiral. The central bulge is prominent, exhibiting a smooth, yellowish hue. The spiral arms are somewhat flocculent, showing a patchy distribution of bluer regions, suggestive of ongoing star formation. The arms are not tightly wound and appear somewhat disrupted. There is evidence of faint tidal features or distortions emanating from the main galactic body, particularly in the form of diffuse extensions, hinting at a possible recent or ongoing interaction or merger. Overall, the morphology points to a system that is neither a perfectly formed spiral nor a completely irregular galaxy, indicating a state of transition or disturbance.
