The galaxy presents a somewhat elongated morphology, appearing roughly elliptical in shape. Its core region exhibits a concentrated luminosity with a yellowish-golden hue, suggestive of an older stellar population. Surrounding this central region is a more diffuse, less intense outer halo of similar coloration. 

Embedded within the galaxy's overall structure are several distinct, brighter nodes or regions which could be star forming regions or obscured background objects. These nodes appear more yellow in color. The overall appearance implies a merging event in the recent or ongoing past, and displays possible signs of minor disturbance to the shape of the host galaxy.
