The galaxy presents as a centrally concentrated, smooth object. The light distribution appears largely elliptical, trending towards a spheroidal shape rather than a distinctly flattened disk. A core region exhibits a yellowish-white hue, suggesting an older stellar population dominating its composition, though some bluer hints suggest more recent star formation is possible. There's a gradual fading of color and luminosity moving outward from the core, with the outer regions displaying a more subdued, bluish tint, indicating a younger population of stars at a further distance from the galactic center. No spiral arm structure or prominent dust lanes are discernible, consistent with a relatively undisturbed morphology.
