This galaxy presents a somewhat elongated, elliptical morphology. The core region exhibits a bright, concentrated luminosity, suggesting a high density of stars. Moving outwards from the center, the light intensity gradually diminishes, forming a diffuse halo. The color gradient transitions from a yellowish hue in the central bulge to a slightly bluer tint in the outer regions, possibly indicating younger stellar populations in the disk or faint spiral arms. The overall structure appears relatively smooth and undisturbed, with no obvious signs of recent major mergers or tidal interactions. The elongated shape indicates that the galaxy is not perfectly spherical, hinting at a more complex formation history.
