The galaxy appears to be undergoing a merger, or at least a significant gravitational interaction, with another galaxy. The primary body exhibits a smooth, elliptical morphology with a central bulge that transitions gradually into a more diffuse halo. The core is a vibrant yellow, which indicates an older stellar population likely dominating the region. Towards the periphery, a slight blue tinge is visible, suggesting the presence of some younger, hotter stars, although star formation activity appears relatively subdued overall. A smaller, bluer companion galaxy is situated in close proximity. The blue color signifies recent or ongoing star formation. There are hints of tidal disturbances or faint extensions in the galaxy's outskirts. Overall, the system presents a disturbed morphology, likely a consequence of the interaction between the two galaxies.
