The galaxy appears as a somewhat elliptical, disc-shaped structure, viewed at a moderate inclination. The central bulge is prominent and displays a yellowish-orange hue, possibly indicating an older stellar population. The disc exhibits a blend of colors, with inner regions showing a yellow-green tint transitioning to a bluer, fainter outer region, suggesting on-going star formation. There is a slight irregularity to the overall shape, possibly due to gravitational interactions or internal disturbances. The galaxy does not appear to be undergoing a major merger, although subtle asymmetries indicate the possibility of a minor disturbance. Overall, the galaxy is characterized by a mix of features typical of both elliptical and spiral galaxies.
