The galaxy presents a largely smooth, elliptical morphology. A central bulge region exhibits a concentrated, yellowish-white hue, suggesting a population of older stars. Moving outwards from the bulge, there's a subtle transition to a fainter, slightly bluer halo, possibly indicating the presence of younger stellar populations or some ongoing star formation, although not dominating the overall light. The galaxy appears generally undisturbed, with no obvious signs of recent major mergers or tidal interactions. The shape is moderately elliptical; it is not perfectly spherical and deviates from a disk shape, with an intermediate ellipticity. Any spiral arms, if present, are either tightly wound or obscured by the viewing angle and distance, appearing mostly featureless in this image. Overall, the galaxy appears as a fairly well-defined and relatively quiescent system, with an estimated stellar mass likely within the range of a typical galaxy.
