The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that emits strongly across the visible spectrum, appearing yellow-white in composite color. The light suggests a population of older stars. The isophotes appear mostly circular. There is little evidence of spiral arm structure or significant dust lanes. A faint blue halo is visible. Overall, the galaxy's light is quite evenly distributed, with no major indications of recent mergers or tidal interactions. The galaxy appears relatively isolated, suggesting a fairly relaxed evolutionary history.
