The galaxy presents an elliptical morphology, with a smooth, centralized light distribution that lacks prominent spiral arm structures. The core region exhibits a high degree of luminosity, appearing concentrated and nearly spherical. Radiating outward from the core, the galaxy gradually fades in intensity, maintaining a consistent, albeit less intense, light profile. The overall color index suggests an evolved stellar population, giving a yellowish-orange tint. There is little indication of ongoing major merger activity or significant tidal disturbances in its immediate vicinity. The galaxy is somewhat rounded, with a smooth appearance. There are no obvious signs of spiral arms or intense star formation regions within the galaxy.
