The galaxy presents an irregular morphology, with noticeable disturbances in its structure, indicating a potential ongoing or recent interaction or merger event. Two distinct, yet connected, components are visible. One component displays a somewhat smoother, elliptical appearance, while the other exhibits a more diffuse and elongated structure. The elliptical component appears to be the dominant mass.

The overall color profile suggests a mix of stellar populations. The central region shows a redder hue, which could be attributed to older stars. Conversely, bluer regions are present, particularly within the elongated structure.

There appears to be a dust lane obscuring parts of the galaxy. There is also a suggestion of tidal tails extending outwards.
