The galaxy presents as a largely smooth, elliptical-like structure, with a concentrated central bulge. The core exhibits a yellowish-orange hue, indicating a population of older stars. Fainter, diffuse, bluish regions extend outward from the central region, possibly suggesting areas of more recent, albeit limited, star formation. The overall form is fairly regular, lacking strong evidence of recent major mergers or tidal disturbances, although minor irregularities in the outer regions cannot be ruled out due to the image resolution. The galaxy appears relatively isolated, which would support this hypothesis.
