The galaxy presents as a largely smooth, elliptical structure. It exhibits a concentrated central bulge, which appears approximately circular. There is a notable absence of clearly defined spiral arms or dust lanes within the visible spectrum. The light profile appears to gradually fade from the core outwards without any discrete features. The overall color is yellowish, with a slight red shift, which potentially indicates an older stellar population and subdued star formation activity. There is no obvious morphological evidence of ongoing or recent major mergers. Any disturbances appear minor if present at all.
