The galaxy appears as a centrally concentrated, elliptical-like structure. It exhibits a smooth, diffuse morphology with a high degree of central luminosity. There is no apparent spiral arm structure or significant dust lane presence. The color gradient suggests a population of older stars, with a redder hue dominating the galaxy's overall appearance. The elongated shape suggests the system is not perfectly spherical but rather ellipsoidal. There are no indications of active galactic nuclei activity, or ongoing major merging events. Minor disturbance features appear possible.
