The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The core exhibits a distinct yellowish-orange hue, suggesting a population of older stars. Surrounding the core, there's a fainter, diffuse halo that extends outwards. Faint spiral arm structures are visible, but they are not well-defined, indicating a possibly more evolved or disrupted disk. The galaxy's overall shape is neither perfectly round nor highly elongated, existing somewhere in between. There are some signs of minor asymmetry or disturbances, but no obvious major merging events are apparent in this image. Star formation is low.
