The galaxy presents as a luminous, yellowish object, approximately elliptical in shape. It displays a centrally concentrated light profile, suggestive of a prominent bulge. The overall color indicates an older stellar population, with fewer young, massive stars. Fainter, bluer regions are tentatively observed in the surrounding disk, indicating the presence of some ongoing star formation. The galaxy appears relatively smooth and undisturbed, lacking clear signs of recent major merger activity, however some minor disturbances may be present. The galaxy appears to be somewhat inclined from our point of view. The estimated physical size is ~10 kpc. The galaxy has a notable mass and a low rate of star formation.
