The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The core region displays a bright, yellowish-white hue, suggesting a population of older stars. A diffuse, fainter halo surrounds the central region, gradually fading into the background. No distinct spiral arms or features are discernible within the resolution of the image. There is no apparent evidence of recent merger activity or significant tidal disturbances. The galaxy appears relatively isolated and undisturbed, consistent with a quiescent evolutionary state.
