The galaxy presents as a relatively compact, smooth object with a general elliptical morphology. It exhibits a concentrated central bulge that appears yellowish-white, suggesting an older stellar population. A fainter, bluer halo surrounds the central region, possibly indicating some degree of ongoing or recent star formation. There is no discernible spiral arm structure or distinct dust lanes visible in this image, implying a lack of significant disk component. The galaxy's overall smoothness and concentrated morphology suggests that it may be an early-type galaxy. There are no apparent signs of any ongoing mergers or major tidal disturbances.
