The galaxy presents a discernible disk structure, though with a somewhat indistinct boundary. A central bulge is visible, neither particularly dominant nor absent, appearing to be of moderate size relative to the overall galactic structure. Evident are spiral arm features, though they are not tightly wound. The galaxy does not appear to be undergoing a major merger, though a minor interaction or disturbance is plausible given the slight asymmetry and irregularity in the outer disk. There may be a bar-like structure. It shows no signs of being edge on. The color profile of the galaxy indicates a mix of stellar populations, suggesting on-going star formation. The galaxy does not exhibit a purely smooth morphology; a structured disk dominates, and a merging event is not evident. 
