The galaxy presents a mostly smooth morphology, although subtle features and possible disk-like characteristics may be present within its structure. The shape appears to be somewhat in between round and elongated, tending more toward a round shape. No strong evidence of major mergers is apparent in the image; it appears to be a relatively isolated system.

Color variations are observed across the galaxy. The core region displays a more yellow-red hue while some outer regions tend more blue, suggesting differing stellar populations. The integrated light suggests a moderate star formation rate. The galaxy's estimated size indicates a moderately sized object in terms of its physical extent.
