This galaxy presents a generally smooth appearance with a slight elongation, suggesting an elliptical morphology or a lenticular galaxy observed at an angle. The light distribution is concentrated towards the center, exhibiting a bright, somewhat diffuse nucleus. Moving outwards from the center, the light intensity decreases gradually, though there is some suggestion of a disc-like structure. Subtle color gradients are present, with the central region appearing more yellow. No distinct spiral arms or prominent dust lanes are discernible, which is consistent with a relatively old stellar population. The overall symmetry is largely undisturbed.
