The galaxy presents as a moderately inclined disk system. It exhibits a central bulge region that appears yellowish-white, suggesting a population of older stars. The disk is faintly visible and appears elongated. There are no prominent spiral arm structures discernible in the image; the disk structure appears smooth and relatively featureless. The overall color suggests it is redder, indicating an older stellar population. There is no obvious dust lane visible and no evidence of strong active star formation. The galaxy appears fairly undisturbed, showing no indications of major mergers or tidal disruptions. The outer regions appear to fade gradually into the background. The galaxy appears to be an elliptical. 
