The galaxy presents a morphology that suggests a spiral structure with notable features. There appears to be evidence of a galactic merger or significant gravitational interaction, indicated by a distinct disturbance in its overall form and possible tidal features. The galaxy is face-on, allowing for a reasonable view of its spiral arms.

There is a bright, moderately sized bulge present at the galaxy's center. The spiral arms are discernible, exhibiting a somewhat flocculent structure. These arms appear less tightly wound and lack the grand design often seen in classic spiral galaxies. The color distribution suggests active star formation regions, possibly dominated by younger, bluer stellar populations.
