The galaxy presents as a generally smooth, elliptical morphology. The light profile appears concentrated towards the center, exhibiting a bright, yellowish core. Moving outward from the core, the galaxy shows a gradual decrease in surface brightness. The outer regions display a reddish hue, potentially indicating a population of older stars. There is a slight asymmetry in the overall shape, suggesting a possible minor gravitational interaction or internal disturbance, though no significant tidal features or distinct merging signatures are readily apparent. The galaxy is more elongated than circular. The galaxy is located at a relatively far distance and appears to have a notably suppressed star formation rate.
