The galaxy presents as a centrally concentrated spheroid with a smooth, diffuse light distribution. There is little evidence of distinct spiral arms or a prominent disk. The core region exhibits a yellowish hue, potentially indicative of an older stellar population. The outer regions display a gradient towards slightly bluer colors, possibly suggesting some ongoing, but limited, star formation. There are some minor indications of tidal disturbance, but no major signs of a merger. The overall morphology appears largely undisturbed and relatively evolved.
