This galaxy presents as a somewhat elongated, elliptical structure. Its core exhibits a bright, concentrated luminosity, suggesting a high density of stars in the central region. The overall color appears to be yellowish-white, which may indicate an older stellar population with fewer hot, young stars. The galaxy’s light distribution is relatively smooth, with no obvious spiral arm structures or significant dust lanes visible. The outer edges of the galaxy fade gradually into the background, indicating a less dense distribution of stars at the periphery. There may be a slight asymmetry in the shape, but it appears largely undisturbed with no obvious signs of a recent major merger event.
