The galaxy presents as a spiral type, exhibiting a well-defined disk structure. There is a noticeable central bulge, with a brighter yellow hue compared to the outer regions of the disk. The spiral arms are tightly wound and appear relatively smooth, lacking significant clumpy star-forming regions discernible at this resolution. The galaxy's light profile is moderately concentrated. The overall color index suggests the presence of a mix of stellar populations, with a bias towards older stars in the central bulge. There is evidence of a possible minor interaction or merging event, with some asymmetry or distortion. There may be some dust lane features obscuring parts of the disk. 
