The galaxy presents as an elliptical morphology, exhibiting a predominantly smooth structure. It possesses a concentrated central bulge, which emits a yellowish hue indicative of an older stellar population, and suggesting lower levels of current star formation. The overall shape appears to be of intermediate ellipticity. There is subtle evidence of minor disturbance in the outskirts of the galaxy, but it appears largely undisturbed. The galaxy's angular size appears relatively small, suggesting it is at a considerable distance. 
