The galaxy presents a disk-like morphology, viewed at a significant inclination. A prominent central bulge is visible, appearing relatively bright and concentrated. Spiral arm structures are present, but their morphology is somewhat indistinct, possibly due to the viewing angle or intrinsic properties of the arms themselves. The winding of these arms appears relatively tight across a substantial portion of the disk. The galaxy does not show obvious signs of major mergers or significant tidal disturbances, though minor irregularities cannot be ruled out. The overall color suggests a mix of stellar populations, with the central bulge exhibiting a yellower hue, indicative of older stars, and the disk showing bluer regions suggestive of ongoing star formation.
