The galaxy appears as a fairly smooth, elliptical object with a concentrated central bulge. The light distribution suggests a relatively old stellar population, with a yellow-orange hue dominant. The galaxy exhibits a somewhat elongated shape, deviating slightly from perfect circularity. There is little evidence of spiral arms or significant dust lanes, further supporting a classification toward the elliptical end of the Hubble sequence. The outer regions fade gradually into the background sky, suggesting a lack of ongoing, intense star formation in the outer disk. Overall, the galaxy presents as a well-established, relatively quiescent system. There is no evidence of any major mergers or tidal disruptions that could otherwise be seen in the image.
