This galaxy presents as a spiral galaxy, exhibiting a disk-like structure with a noticeable bulge at its center. The spiral arms are quite tightly wound, creating a somewhat flocculent and less distinctly defined pattern, and appear to have a moderate number of arms, though a precise count is challenging. The color gradient suggests a distribution of stellar populations; the central bulge exhibits a yellowish hue, potentially indicating older, redder stars, while the spiral arms show a bluer tint, which would indicate younger, hotter stars and ongoing star formation. The galaxy is inclined relative to our line of sight, and we are viewing it at an angle. There is no visual evidence of any major mergers or tidal disturbances and no clear bar structure is discernible.