The galaxy presents as a relatively compact, luminous object. It exhibits a somewhat smooth, elliptical morphology, though subtle structural features hint at possible disturbances. Color gradients are present, with a bluer core and a redder halo. This suggests a distribution of stellar populations, potentially with younger, hotter stars concentrated in the central region and older, cooler stars populating the outer regions. Faint tidal features are present, indicating past interaction with another galaxy. These features could represent remnants of a minor merger or gravitational disturbance. Overall the galaxy appears to be in the process of merging with one or more other galaxies.
