The galaxy presents as a relatively compact object with a discernable core. Its morphology suggests some level of disturbance, potentially indicating an ongoing or recent interaction or merging event. There is evidence of asymmetry in its structure. A faint, extended halo or tidal tail is present, extending outwards from the main body of the galaxy. The overall color profile indicates a mix of stellar populations, with a central concentration that has a blue tinge with an increasing red tinge near the trailing tail.
