The galaxy presents a generally smooth, elliptical morphology. The light is concentrated towards the center, forming a bright, dense core. A diffuse halo extends outwards from this core, gradually fading into the background. The overall color is a yellow-orange hue, suggesting an older stellar population with relatively little ongoing star formation. No distinct spiral arms or prominent dust lanes are discernible. The galaxy exhibits a high degree of circularity, appearing nearly spherical. There is no evidence of major mergers or significant tidal disturbances affecting its structure, though there seems to be a slight asymmetrical luminosity distribution in the outer regions.
