The galaxy exhibits a diffuse morphology. The overall form is not clearly defined, with the structure appearing somewhat amorphous. There is no prominent central bulge or spiral arm structure immediately visible. A hint of tidal tails can be observed at the edges of the galaxy suggesting gravitational interactions. The primary color appears to be reddish, with a slight contribution of blue light in the outer edges. This may indicate a relatively older stellar population, but some ongoing star formation is possible. There is likely ongoing merger activity or recent merger that has disturbed the main structure. The overall galaxy appears relatively smooth. The central region seems to be compact and has a relatively brighter intensity.
