The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that gradually fades into a more diffuse halo. A subtle color gradient is observed, with the core appearing slightly more yellow/red, suggesting an older stellar population concentrated toward the center, and bluer colors at the edges. No distinct spiral arms or significant dust lanes are visible. There is very slight evidence of tidal disturbances or faint features suggestive of minor mergers, but generally this is not an actively merging system. It's a galaxy with a red shift indicating it is not a local galaxy and is at a considerable distance from us. 
