The galaxy appears as an elliptical, centrally concentrated object. The core exhibits a bright, relatively homogenous glow, suggesting a substantial population of stars or active galactic nucleus activity. Moving outwards from the center, there is a noticeable transition to a fainter, extended halo. This halo appears somewhat asymmetrical, with a slightly irregular shape, potentially indicating past or ongoing interactions. There is no clear evidence of spiral arms or a well-defined disk structure. Faint color variations are visible within the galaxy; the central region appears bluish-white, transitioning to greenish-yellow in the outer parts of the halo. This color variation could be due to differences in stellar populations or dust content. Overall, the galaxy presents as a relatively compact object with a smooth profile, although subtle morphological disturbances cannot be ruled out. The galaxy shows signs of possible merger activity in the recent past, with some distortion visible in the outer regions.
