The galaxy presents a largely smooth morphology with a centrally concentrated light profile. The object has a generally elliptical shape, tending toward round. A faint, diffuse halo or envelope appears to extend outward from the central region, displaying a slightly disturbed structure on one side. There is evidence of asymmetric features, suggesting a possible minor interaction or past merger event. Color gradients are visible, with a central, yellowish core. The outer regions of the galaxy display bluer hues, consistent with the presence of a younger stellar population. Overall, the galaxy exhibits characteristics consistent with an elliptical type, though some observed disturbances hint at a more complex evolutionary history.
