The galaxy presents a disk-like morphology with a substantial bulge. The bulge appears centrally concentrated and exhibits a smooth, relatively featureless profile, with a moderate size relative to the entire galaxy. Spiral arm structures are visible within the disk. These spiral arms are somewhat tightly wound and appear to extend from the central bulge outwards. There are at least two arms visible, with hints of other fragmented spiral substructures present in the disk. The color distribution suggests a mix of stellar populations, with bluer regions likely indicating areas of ongoing star formation, particularly within the spiral arms. The overall shape of the disk suggests a mild inclination relative to the observer's line of sight. The galactic disk shows no obvious signs of major merger activity or significant tidal disturbances.
