The galaxy presents a largely smooth, elliptical morphology. It has a prominent central bulge, exhibiting a concentrated luminosity profile. The galaxy is not perfectly spherical, deviating slightly towards an elongated shape, but is not significantly cigar-shaped. The color distribution indicates a dominant population of older stars, contributing to a yellowish hue, especially within the central region. There's some indication of bluer regions, suggesting possible ongoing, though likely subdued, star formation, though this could also be an artifact of the image. Overall, the galaxy shows no signs of major disturbances or recent mergers, appearing relatively isolated and evolved.
