The galaxy presents as a smooth, centrally concentrated object, exhibiting an elliptical morphology. The light distribution is characterized by a dominant spheroidal component with a significant red color index. The overall shape is elongated, with an axial ratio suggesting a moderate degree of ellipticity. There is no discernible spiral arm structure or prominent dust lanes. The light profile appears relatively uniform, lacking significant surface brightness fluctuations or tidal features, indicating a dynamically relaxed system. Faint blue emission is present in the outer reaches of the halo, suggesting some star formation activity in the galaxy, albeit at a low rate.
