The galaxy presents as a lenticular or possibly an elliptical galaxy due to its generally smooth appearance. The light is concentrated towards the center, exhibiting a radial profile that gradually fades towards the edges, but it is slightly elongated. It appears as a cigar shape. There is no clear evidence of spiral arm structures or significant dust lanes that would indicate active star formation within the galaxy. The color of the galaxy is a relatively uniform off-white, which could be indicative of an older stellar population. The galaxy exhibits minimal signs of ongoing merger activity, disturbances, or other significant gravitational interactions. The overall appearance of the galaxy suggests a relatively evolved system that may have exhausted most of its gas supply for star formation. The faintness of the galaxy suggests that it is at a considerable distance from the observer.
