The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a somewhat elliptical shape, although it leans toward being more in between elliptical and round. There appears to be no strong evidence of spiral arm structure or a prominent disk component. There is no presence of a strong bar feature. The galaxy's color suggests a relatively old stellar population, and based on the lack of clear disturbances, this galaxy does not appear to be currently undergoing any major mergers, although minor disturbances cannot be ruled out.
