The galaxy presents as an elliptical morphology, characterized by a generally smooth light distribution. There is a high concentration of light toward the center, which declines gradually outwards. There appears to be an absence of spiral arm structures. The shape of the galaxy appears elongated rather than circular. Color gradients across the galaxy suggest a population of older stars, especially in the central region, which exhibits a yellow-orange hue. The outer regions appear slightly bluer, potentially indicating more recent star formation activity, albeit at a low rate. No significant tidal features or indications of major merging events are observed in the immediate vicinity.
