The galaxy exhibits a generally elliptical morphology. There is a bright, concentrated central region, suggesting a possible galactic nucleus. Extending outward from the center is what appears to be a disk component, though it may be difficult to distinguish. The disk is brighter in some regions than others, perhaps showing some spiral arm structure. The color profile of the galaxy varies. The central region appears to be white, perhaps indicating a diverse population of stars or significant star formation. The disk shows color variations, shifting from redder hues on one side to bluer tones on the other, potentially a sign of differential stellar populations or dust obscuration. The overall structure is somewhat disturbed, showing asymmetry, and there is some evidence for tidal features or minor irregularities, suggesting the possibility of past or ongoing interactions with another galaxy. 
