The galaxy presents a generally smooth and elliptical morphology. The light distribution appears centrally concentrated, exhibiting a bright core that diffuses outwards. There is a slight elongation, suggesting it is not perfectly spherical. The galaxy displays a color gradient, with the core appearing bluer compared to the outer regions, which exhibit a redder hue. No distinct spiral arms or bar structures are discernible. The overall appearance is consistent with a relatively evolved system. The lack of significant morphological disturbance indicates it has likely not undergone a recent major merger. The light is fairly compact with no dust lanes.