The galaxy presents as a centrally concentrated, luminous structure. It appears relatively smooth in morphology, lacking prominent spiral arms or a distinct disk. The light profile suggests an elliptical or lenticular galaxy type. The core region shows a yellowish-white hue, potentially indicating a population of older stars. Fainter, diffuse light extends outwards from the core, exhibiting a subtle gradient in intensity. There is a minor asymmetry in the light distribution, possibly suggesting a weak tidal interaction or past merger event, though overall the galaxy appears largely undisturbed. The color is indicative of a red sequence galaxy, likely with suppressed star formation.
