The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a largely elliptical morphology, with an intermediate degree of ellipticity, showing it is somewhat in between round and cigar shaped. There is no clear evidence of a prominent disk structure or spiral arms. The galaxy's light profile suggests minimal disturbance from ongoing or recent major mergers. The central region appears bright, while the outer regions fade gradually into the background sky, the colors seem to indicate there is a higher concentration of older stars, and little presence of newly forming stars.
