The galaxy presents as a centrally concentrated, elliptical-like object with a smooth, diffuse morphology. The core region exhibits a yellowish-white hue, potentially indicating an older stellar population. Moving outwards from the core, the color shifts to a bluish-green, possibly signifying a presence of younger, hotter stars or regions of ionized gas. There is no apparent spiral arm structure or defined dust lanes visible within the galaxy's disk. The overall light distribution is relatively uniform, with a gradual decrease in brightness towards the outer edges. The galaxy appears relatively undisturbed, with no obvious signs of recent major merger activity or tidal distortions. The elongated shape suggests it is somewhere between a round elliptical and a cigar-shaped elliptical galaxy. Some minor disturbances might be present but these are not too disruptive to the galaxy's overall shape.
