The galaxy appears to be a relatively smooth, elliptical or lenticular type. It presents a slightly elongated shape, deviating from perfect circularity. The color gradient suggests a concentration of older stellar populations. The core region exhibits a yellowish hue, indicative of evolved stars. No prominent spiral arms or dust lanes are discernible. The galaxy appears largely undisturbed, lacking obvious signs of ongoing mergers or tidal interactions. It is generally homogenous in color, with subtle variations in brightness that could point to minor structural features.
