The galaxy presents as an ellipsoidal structure with a moderately high degree of central concentration. Its overall color is yellowish-orange, suggestive of an older stellar population with a relatively low rate of on-going star formation. The galaxy's morphology is neither perfectly spherical nor highly elongated, displaying a somewhat intermediate shape. There appear to be some minor disturbances, but not major asymmetries that would obviously suggest an on-going merging event. However, a possible interaction with a smaller neighboring galaxy, a dwarf satellite, is suggested, a fainter companion appearing slightly offset from the primary galaxy's nucleus.
