The galaxy presents a generally smooth, elliptical morphology. Its core exhibits a bright, concentrated luminosity, transitioning outwards to a more diffuse halo. The galaxy displays a slight yellowish hue in its central regions, which may suggest an older stellar population. Moving outward from the center, the galaxy exhibits a faint bluish-white color, which may be suggestive of younger stars and low levels of star formation. There are no obvious signs of spiral arms, bars, or major disturbances in the galaxy's overall structure. It appears relatively isolated, with no immediate indications of ongoing mergers or tidal interactions. The galaxy's apparent roundness suggests that it is viewed close to face-on.
