The galaxy presents a mostly smooth, elliptical morphology. The light profile appears centrally concentrated with a gradual decrease in intensity outwards. It displays a yellow-reddish hue, suggesting a relatively older stellar population with lower ongoing star formation. The overall structure exhibits a high degree of symmetry, with no obvious signs of spiral arms or significant dust lanes. It seems to show a minor disturbance, the nature of which is difficult to determine given the resolution. It may show evidence of recent or ongoing galaxy interaction or merger. The galaxy is likely a massive system.
