The galaxy presents as a relatively smooth, elliptical-like structure. Its color profile suggests a population of older stars, with a general yellowish-red hue dominating the galactic body. There may be faint signs of a disk-like structure but this is not definite from the color. The galaxy appears to be an isolated system, without evidence of major tidal disturbances or interactions with other galaxies in its immediate vicinity. It is moderately compact, with a relatively concentrated light profile, lacking the presence of prominent spiral arms or regions of intense star formation. Given the morphology, it is likely the galaxy is relatively evolved.