This galaxy appears to be a merging system, or potentially two interacting galaxies. There are two primary concentrations of light, suggesting two distinct galactic nuclei. Both components exhibit a smooth, elliptical-like morphology with no obvious spiral arm structure visible. The light from each component is concentrated toward the center, with a gradual decrease in intensity towards the outer edges.

The color gradient suggests a moderate amount of star formation may be occurring. Yellowish-red hues are visible within each component, possibly indicating the presence of older stellar populations and dust. There also appears to be a subtle bridging of material between the two components, implying gravitational interaction and tidal forces at play. This could be gas and dust being pulled between the two galaxies.
