The galaxy presents as a spiral type, though the orientation is oblique, offering only a limited view of the disk structure. Evident spiral arms are somewhat flocculent in appearance and not tightly wound. The central bulge is prominent and appears relatively large compared to the overall size of the galaxy, exhibiting a yellowish hue indicative of an older stellar population. There is a subtle color gradient from the center outwards, with the disk showing bluer regions suggestive of ongoing star formation activity. No obvious bar structure is discernible. The overall appearance suggests a galaxy undergoing modest star formation with a relatively high mass. No significant signs of tidal disturbance or recent major mergers are visible. The galaxy's light distribution indicates a moderately concentrated morphology.
