The galaxy presents as a somewhat compact and moderately luminous system with a smooth, centrally concentrated morphology. There is evidence of a slight disk-like component, though it is not sharply defined. The central bulge appears dominant, exhibiting a yellow-white hue, suggesting a relatively older stellar population. The outer regions display a bluer tint, indicating the presence of younger, hotter stars, potentially tracing regions of recent star formation. There are minor irregularities in the outer regions and the galaxy appears somewhat disturbed. These irregularities could be signs of a possible minor interaction or merger event. The overall light distribution is fairly uniform, with no prominent spiral arms or other distinct features immediately apparent.
