This galaxy appears to be in the process of merging or experiencing a significant gravitational interaction. The primary body of the galaxy presents a smooth, somewhat amorphous structure with an elliptical-like shape. There appears to be a central concentration of light, suggesting a possible core or nucleus. A secondary, slightly less luminous component is visible and connected to the main body by what appears to be a stellar bridge or tidal arm. There might also be indications of a faint tidal tail extending outward. The color profile indicates an older stellar population, with the dominant hues being yellowish-orange. There is little evidence of significant ongoing star formation, based on the lack of blue or UV emissions.
