The galaxy presents as a centrally concentrated object with a smooth, diffuse halo. The core exhibits a yellowish hue, possibly indicating an older stellar population. The overall morphology appears largely undisturbed, with a slight elongation suggesting a possible transition between elliptical and lenticular types. There is a hint of redder emission off to the side, possibly indicative of an area of localized star formation or a region of dust obscuration. The galaxy appears relatively isolated, lacking obvious signs of tidal interactions or close companion galaxies. The estimated size of the galaxy indicates it is a moderately large galaxy, in terms of its effective radius.
