This galaxy presents as a generally smooth and rounded structure. The core exhibits a concentrated, bright luminosity. The surrounding halo appears less luminous, with a gradual decline in brightness moving outward from the central region. There is a very subtle blue tinge on one side of the halo. Based on its morphology, a low star formation rate might be present, with some evidence of a population of older stars dominating the galaxy's stellar content. There does not appear to be any significant disturbance to the overall structure. The galaxy does not appear to have any signs of spiral arms or a pronounced disk structure.
