The galaxy presents as an elliptical morphology with a relatively smooth texture. It exhibits a concentrated central bulge with a yellow-gold hue, suggesting an older stellar population. The galaxy appears moderately rounded, with a slight elongation along one axis. There is little to no evidence of spiral arms or significant disk features. A faint blue-ish halo surrounds the central region, possibly indicating a younger, more dispersed population of stars or some ongoing star formation at the edges. The overall structure implies a system that is likely dynamically relaxed, with minimal signs of recent major mergers or disturbances.
