The galaxy presents a generally smooth morphology, with a high degree of central concentration. The shape approximates a near-circular ellipse. Faint, somewhat indistinct, features are present, suggestive of a possible disk component or minor asymmetries, yet the overall appearance remains largely spheroidal. Color gradients are evident, exhibiting a central region with enhanced yellowish tones and a gradual transition to a bluer, more diffuse periphery. The lack of strong color variations across the disk implies a relatively homogenous stellar population. There is a subtle hint of disturbance in its structure. The low star-formation rate is consistent with an older stellar population.
