This galaxy appears to be a relatively smooth, elliptical system. Its overall morphology suggests a spheroid-dominated structure, with minimal evidence of spiral arms or significant disk features. The galaxy exhibits a centrally concentrated brightness profile, indicative of a dense core. The observed color gradient, from the core to the outer regions, seems to be relatively uniform. There are some suggestions of low-level disturbances, but the galaxy appears mostly relaxed. At its distance, there are hints of ongoing, but minimal star formation activity. The galaxy's red color suggests that it consists primarily of an older stellar population.
