The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated bulge that dominates its overall light profile. The luminosity fades gradually from the core outwards. The galaxy displays a slightly elongated shape, somewhere between round and cigar-shaped. There are no readily apparent spiral arms or distinct dust lanes visible. The light distribution is consistent with an older stellar population; the overall color suggests the presence of evolved stars. There are no obvious signs of ongoing major merger activity or strong tidal disturbances, although minor disturbances cannot be ruled out due to the image quality.
