The galaxy presents as a single, relatively smooth, centrally concentrated light source. The object exhibits a high degree of circular symmetry. There is no strong evidence of spiral arm structure or a prominent disk. The light profile appears to be fairly uniform and diffuse, with a gradual decline in intensity from the center outwards. A significant population of older stars is suggested by its color. Visual assessment doesn't reveal any obvious signs of ongoing major mergers or significant tidal disturbances. The data suggest that it is a quiescent system with a suppressed star formation rate.
