The galaxy exhibits a disk-like structure, with a significant central bulge. The spiral arms are tightly wound. The galaxy displays a range of colors, with a yellowish hue near the core, likely indicative of older stellar populations, transitioning to bluish tones in the outer regions, potentially suggesting more recent star formation. There does not appear to be a strong presence of a bar-like structure within the central region. There is no signs of any major merger events happening.