The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated luminosity profile. The core exhibits a yellowish-white hue, suggesting a population of older stars. The overall shape is elongated, with a major axis roughly twice the length of the minor axis. There is a slight indication of a very faint disk, but no spiral arm structures are discernible. The red color index is slightly high, supporting this hypothesis. A lack of substantial dust lanes is observed. There is a faint blue patch on one end of the galaxy indicating possible star formation.