This galaxy presents as a somewhat disturbed system, potentially undergoing a minor merger event. The primary galactic body exhibits a concentrated central bulge with a diffuse, extended halo. The morphology deviates from a pure elliptical classification, suggesting the presence of a flattened disk component. This component displays hints of spiral arm structures but are not fully defined. Patches of bluer light are scattered throughout the galaxy, likely indicating regions of ongoing star formation, although these are not particularly prominent. A tidal tail is visible extending upwards from the main body, suggestive of gravitational interaction. Overall, the galaxy's color is predominantly reddish-yellow, indicating an older stellar population.
