The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth and concentrated light profile with minimal discernible structure. The luminosity is concentrated towards the center, fading gradually outwards. The morphology appears mostly rounded. There's no apparent spiral arm structure or significant dust lane obscuration, indicating it may be a more evolved system. The color appears moderately red. This is consistent with a population of older stars and a suppressed rate of star formation. There's no obvious sign of ongoing merger activity or strong tidal disturbances. 
