The galaxy presents as a luminous, elliptical structure. It exhibits a smooth, featureless morphology, lacking prominent spiral arms or a well-defined disk. The light is concentrated towards the center, suggesting a dense galactic nucleus. The galaxy's shape is largely spheroidal, appearing quite round, with only slight deviations towards an elongated form. There is no clear evidence of active galactic nuclei activity, such as jets or strong emission lines, based on its color and morphology. Additionally, there is no clear evidence of major disturbances or ongoing mergers, though a minor interaction cannot be entirely ruled out given the limited resolution of the image. The color suggests the presence of an older stellar population.
