The galaxy appears to be composed of a primary, centrally located component and a secondary component to its left. The primary component exhibits a smooth, centrally concentrated light distribution, indicative of an elliptical morphology. The secondary component appears more diffuse and disc-like, suggesting a spiral or irregular morphology.

The color of the primary component is predominantly yellow-orange, potentially indicating an older stellar population with lower levels of active star formation. The secondary component exhibits a slightly bluer hue, suggesting the presence of younger, hotter stars and possibly ongoing star formation, although at a relatively low rate.

There is evidence of tidal interaction or merger activity due to the apparent close proximity and morphological distortion.
