This galaxy presents as a relatively smooth, elliptical-like structure. The light distribution suggests a high degree of central concentration, with brightness decreasing gradually towards the outer edges. The galaxy's color is generally yellowish to white, indicating a stellar population that is dominated by older stars. There is little to no evidence of spiral arms, dust lanes, or prominent star-forming regions. The overall appearance suggests a galaxy that has largely exhausted its supply of gas and dust, and has a low star formation rate. There is no noticeable signs of a merger.
