The galaxy presents a largely smooth morphology, suggesting it is potentially an elliptical or lenticular type galaxy. The galaxy exhibits a generally round shape, leaning slightly more towards an "in between" circularity than a perfectly circular appearance. It presents with a prominent central bulge of concentrated light, appearing yellowish-orange in color. This core is significantly brighter than the surrounding galactic halo. There are no readily apparent spiral arms or significant dust lanes visible in this image. The relatively smooth texture and yellow-orange hue indicates an older stellar population and a low rate of ongoing star formation. There is no obvious evidence of major mergers or significant tidal disturbances.
