The galaxy appears as a generally smooth, elliptical-like structure. Its core exhibits a concentrated, bright yellowish-white hue, suggesting a higher density of older stars. This central region transitions smoothly to a more diffuse, outer halo. There's a slight elongation or cigar-shaped morphology, indicating it is not perfectly spherical. Minimal evidence of distinct spiral arms or irregular features are observed. The colour gradient from the center to the outer regions may indicate differing stellar populations and ages. Overall, the galaxy appears relatively undisturbed, with no signs of major mergers or significant tidal interactions. There are suggestions of minor disturbances.
