The galaxy appears as an elliptical system with a smooth, diffuse morphology. Its light profile suggests a central bulge that gradually fades outward into a more extended halo. There is little to no evidence of spiral arm structure or significant dust lanes. The galaxy exhibits a yellowish-white color, which is indicative of an older stellar population with lower rates of star formation. There may be some minor disturbances to its shape, but the galaxy appears mostly unperturbed and not undergoing any major merger events. The galaxy is slightly oblong, somewhere in between round and cigar shaped.
