The galaxy presents an elliptical morphology, appearing elongated along its major axis. The light distribution is smooth and centrally concentrated, with a gradual decrease in surface brightness towards the outer edges. There is a subtle color gradient visible, with the central region exhibiting a slightly redder hue compared to the outer regions, which appear bluer. This could suggest a difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars located further out. There is no evidence of spiral arms, a prominent disk, or significant dust lanes within the galaxy. The overall structure suggests a relatively undisturbed system, with no signs of recent major mergers or tidal interactions.
