The galaxy appears to be an elliptical galaxy, with a smooth, round morphology. It exhibits no distinct spiral arm structures. The light distribution is centrally concentrated, fading gradually towards the edges. A hint of disturbance is visible in the morphology of the galaxy, it may be interacting with another galaxy, or perhaps a recent merger event has occurred, though the overall structure is not significantly disrupted. The galaxy's red color suggests an older stellar population, with a relatively low star formation rate.
