The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge that transitions smoothly to a fainter, more diffuse halo. There is a slight elongation, indicating a deviation from a perfectly circular shape, though it appears mostly round. No distinct spiral arms or dust lanes are discernible within the image. The color gradient suggests an older stellar population, with a yellowish hue dominating the overall appearance. Star formation is likely minimal or absent. There's no obvious evidence of active galactic nuclei or significant ongoing interaction with other galaxies. It appears to be a relatively isolated and evolved system.
