The galaxy presents a smooth, elliptical morphology. It exhibits a high degree of central concentration, with the luminosity gradually decreasing from the core. The galaxy appears nearly circular, showing only a slight flattening. There is no evidence of spiral arms or a prominent disk structure. The color profile suggests a dominant population of older stars. No active galactic nucleus or significant dust lanes are apparent. Overall, this galaxy appears to be a relatively quiescent elliptical galaxy, consistent with little recent star formation activity.
