The galaxy presents a face-on orientation relative to our line of sight, revealing a discernible spiral structure. The central bulge appears moderately prominent and exhibits a yellowish-red hue, potentially indicating an older stellar population. Two spiral arms are clearly visible, tracing a path around the central bulge. The arms display a moderate winding pattern, neither tightly wound nor loosely defined. Patches of bluer light are interspersed along the spiral arms, suggesting regions of active star formation. There is a possible bar structure apparent. No significant morphological disturbances or signs of ongoing major mergers are evident.
