The galaxy presents a smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that gradually fades into the outer regions. The shape is not perfectly circular, appearing somewhat elongated or oval. There is no evidence of distinct spiral arms or a prominent disk structure within the visible spectrum. Faint color variations are apparent, potentially indicating differences in stellar populations or dust distribution. Overall, it appears to be a relatively quiescent galaxy with limited ongoing star formation.
