The galaxy appears to be a relatively smooth, elliptical-like structure. Its central region exhibits a bright, concentrated core with a yellowish hue, suggesting a population of older stars. The light intensity gradually decreases outward from the core towards the periphery. There is a slight elongation, as the galaxy is not perfectly circular, hinting at a potentially spheroidal or lenticular shape viewed at a small angle. No distinct spiral arm structures or dust lanes are visible. Faint, diffuse light extends beyond the central region indicating a halo. There's no obvious evidence of recent or ongoing major mergers or tidal disturbances from this image. The morphology suggests a galaxy with a dominant bulge component and a likely low star formation rate.
