The galaxy presents as a somewhat elliptical, yellow-hued object. It is relatively smooth in appearance, exhibiting a centrally concentrated bulge that gradually fades into a fainter outer disk. There is no clear evidence of spiral arm structure, and the overall morphology suggests a relatively evolved system. The axial ratio indicates that the galaxy is not perfectly spherical, but rather has a slight elongation. The light distribution implies a relatively homogeneous stellar population, with little indication of ongoing, widespread star formation. Faint disturbances are present, indicating there may be minor interactions or tidal forces at play. There also may be a merger occurring with the galaxy, though it is not highly disturbed as a result.
