The galaxy presents an elliptical morphology, exhibiting a smooth, concentrated light profile. A bright, centrally located bulge dominates the overall luminosity. The light distribution is not uniform, exhibiting variations in intensity across its structure. There are subtle indications of minor disturbances or irregularities, possibly suggestive of past interactions, though the overall structure appears largely undisturbed. There are no visible spiral arms or prominent disk-like features observed. Color gradients suggest variations in stellar populations or dust content within the galaxy, with the central bulge appearing a yellow-white color, while the outer regions appear more red.
