The galaxy presents as an elliptical morphology, although it shows some slight flattening suggestive of a possible transition between elliptical and lenticular types. Its color profile indicates a dominant population of older stars, with a yellowish hue concentrated towards the center and a subtle blue tinge around its outskirts. This could suggest there is ongoing star formation within its dusty arms. The central bulge is prominent and smooth, with a high concentration of light. The outer regions appear more diffuse, lacking distinct spiral arm structures. There is minimal evidence of tidal disturbances or ongoing mergers. It exhibits an intermediate luminosity. Overall, this galaxy appears to be a massive and relatively quiescent system, consistent with a galaxy that is approaching the red sequence.
