The galaxy presents as an elliptical or lenticular system, exhibiting a predominantly smooth morphology. The central bulge is luminous, appearing yellowish-white, indicative of an older stellar population. A fainter, bluer region extends away from the bulge, possibly suggesting recent star formation or interaction with another galaxy. There appears to be minor distortions or disturbances. The primary body of the galaxy appears largely spheroidal in shape, but there are possible signs of disturbance that suggests it is not completely relaxed. The image quality limits detailed assessment of any spiral arm structures, but the general color gradients and shapes suggest a quiescent or transitioning system.
