The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears largely elliptical or spheroidal with a high degree of roundness. The central region exhibits a brighter, yellowish hue which fades into a slightly redder outer region. There is little to no apparent spiral arm structure or significant dust lane presence based on visible inspection. Evidence suggests that the galaxy is not actively undergoing a major merger, although minor disturbances in its shape can not be entirely ruled out. The galaxy is observed to be a considerable distance away, thus the details of the features are hard to specify. 
