The galaxy presents a generally elliptical morphology with a smooth light distribution. The central region exhibits a concentrated, bright core, indicative of a possible galactic nucleus. Progressing outwards from the core, the intensity of light gradually decreases, exhibiting a somewhat diffuse halo. The colors appear yellowish, indicating the presence of older stellar populations. There is a possible disk-like structure oriented horizontally through the center. There is no evidence of prominent spiral arms or significant dust lanes. The overall appearance suggests a relatively evolved galaxy, potentially undergoing little to no active star formation at the present epoch.
