The galaxy appears to be elliptical in morphology, with a smooth and diffuse light distribution. It is generally round, with a slight elongation. The central region exhibits a high concentration of light, gradually decreasing in intensity towards the outer edges. The galaxy presents a yellow-orange hue, possibly indicating an older stellar population and lower rates of ongoing star formation. There is no evidence of spiral arms, a prominent disk structure, or any major disturbances suggesting a recent merger event. Faint hints of tidal features or minor disturbances may be present, but the dominant visual impression is that of a relatively undisturbed and smooth system.
