The galaxy presents as a relatively smooth, elliptical-like structure. Its core is a bright, concentrated region emitting primarily yellow-white light, suggesting a population of older stars. The light appears to diminish gradually towards the outer edges. There is little evidence of distinct spiral arms or significant dust lanes. The overall structure appears to be largely spheroidal, with an approximate projected diameter of about 5 kiloparsecs. There might be a slight disturbance in its symmetric shape and hints of faint tidal features, but without additional data, this cannot be fully confirmed. The colors suggest a low star formation rate.
