The galaxy presents a generally smooth and elliptical morphology. It exhibits a moderate elongation, appearing somewhat cigar-shaped. The light distribution is centrally concentrated with a gradual decrease in intensity outwards from the core. The central region appears brighter and exhibits a bluer color. The outer regions are less intensely illuminated and demonstrate a redder hue, suggesting older stellar populations. There is no obvious evidence of spiral arms or significant dust lanes. The galaxy does not show any strong signs of tidal disturbances or ongoing merger activity.
