The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge that exhibits a yellowish-orange hue. The outer regions fade into a more diffuse, less defined structure. There's a lack of distinct spiral arms or prominent dust lanes visible. The galaxy appears to be relatively undisturbed, showing no obvious signs of a major merger event or significant tidal disruption. The roundness is elongated, somewhere between round and cigar shaped. The color profile suggests an older stellar population. The absence of strong blue components indicates a comparatively low rate of recent star formation.
