The galaxy presents as a single, moderately luminous object exhibiting a disturbed morphology. The overall form appears elongated, neither distinctly elliptical nor spiral. There is an irregular feature present, giving the impression of an ongoing or recent merger event. Two brighter, somewhat diffuse, yellowish regions are observed on the center, potentially representing the combined nuclei of the interacting galaxies or regions of intense star formation triggered by the interaction. The outer regions display a fainter, bluish glow. While faint, the colors suggest the presence of a younger stellar population. The system lacks a well-defined disk.
