The galaxy appears to be composed of two distinct components. The primary component is a centrally concentrated, smooth, and luminous structure, exhibiting a yellowish-orange hue. This suggests an older stellar population, potentially indicative of an elliptical or lenticular galaxy. The shape appears somewhat elongated but not highly flattened.

A secondary, fainter component is observed nearby. It appears as a more flattened, disc-like structure, with a bluer color in some regions. This could indicate ongoing star formation within this component, possibly a spiral or irregular galaxy. The proximity and morphological distortion suggest a possible gravitational interaction between the two galaxies, though there is no strong visual evidence of tidal tails or bridges.
