The galaxy presents as an elliptical morphology, appearing largely featureless and smooth in structure. The core region exhibits a concentrated luminosity, suggesting a higher stellar density, with a dominant yellowish hue. The light gradually diffuses outwards from the center, forming a less luminous halo. The lack of well-defined spiral arms or dust lanes indicates a predominantly older stellar population and a relatively low ongoing star formation rate, if any. There is no apparent evidence of any major tidal disturbances or ongoing merger events. The galaxy's overall shape is neither perfectly spherical nor highly elongated.
