The galaxy appears as a somewhat rounded, disk-shaped structure with a central bulge. The color distribution suggests ongoing star formation, particularly concentrated in regions within the disk, which presents a bluer hue. There is a central concentration of older stars, likely contributing to the bulge's overall yellower color. Some asymmetry and subtle disturbances in the outer disk are present which could be indicative of possible interactions or mergers. The overall structure suggests a spiral or lenticular galaxy with moderate star-forming activity and a considerable stellar mass.
