This galaxy exhibits a disturbed morphology, indicative of an ongoing or recent merger event. The primary galactic body presents a somewhat amorphous structure, lacking a well-defined spiral arm pattern or elliptical shape. There is a secondary galactic component in close proximity to the primary body. The two components appear to be gravitationally interacting, with tidal distortions potentially visible in the form of faint extensions or bridges of light and dust.

The galaxy displays a range of colors, with a concentration of yellow/orange light in the central regions, which may suggest an older stellar population. Bluer regions are scattered throughout the disk, possibly indicating areas of active star formation. However, the overall color is relatively red, indicating it is not vigorously forming stars. Dust lanes might be present, further obscuring the starlight. The galaxy has a relatively high estimated mass.
