The galaxy presents as a flattened elliptical morphology, exhibiting a moderately smooth appearance throughout its structure. There is evidence of a distinct tidal tail on the right and a possible counter tidal tail on the left, implying a possible recent or ongoing interaction or merger. The core is compact and centrally located, displaying a yellow to red tint. The disk, while smooth, is not featureless, and it is oriented in a way such that we are viewing it close to edge-on. There is a hint of a dust lane visible across the galaxy. There appears to be an elongated, disturbed structure, exhibiting signs of tidal disturbances consistent with a potential galactic merger or gravitational interaction. The outer regions show a more diffuse and irregular structure compared to the central region. Overall, the galaxy's structure suggests a complex evolutionary history possibly shaped by gravitational interactions.
