The galaxy presents as a relatively smooth, centrally concentrated structure, suggesting an elliptical morphology. The core exhibits a yellowish hue, potentially indicative of an older stellar population. There is a subtle color gradient, with a slightly bluer tint towards the outer edges of the galaxy, hinting at the presence of some younger stars or ongoing, albeit limited, star formation. There is a slight distortion in the galaxy. There is a minor disturbance visible in the galaxy, which is likely due to tidal interactions.
