The galaxy presents as a concentrated, elliptical form with a smooth, largely featureless appearance. A bright, yellowish core dominates the central region, indicating a high concentration of older stellar populations. This luminosity appears to gradually decrease outward. Faint extensions of diffuse light are observable at the edges of the galaxy which suggests a halo of older stars. There appears to be slight flattening and deviation from a perfectly circular shape which might be caused by rotation or tidal interactions, but overall, the galaxy is quite symmetrical. There is no evidence of spiral arms or active star-forming regions.
