The galaxy presents an elliptical morphology, exhibiting a smooth, relatively featureless structure. It shows a high degree of central concentration, with the luminosity decreasing gradually outwards from a bright core. There appears to be a slight elongation.

The color is predominantly yellow-orange, which would correspond to a galaxy primarily populated with older stellar populations, indicating a low star formation rate. Traces of light bluer colors are present, particularly in the outskirts, possibly suggesting the presence of some younger stars or regions of limited star formation activity. There is no evidence of spiral arms, distinct dust lanes, or any signs of major disturbances due to mergers.
