The galaxy presents as a dominant, centrally concentrated elliptical or lenticular system with a smooth morphology and an aspect ratio approaching unity, suggesting a near face-on orientation. The light profile decreases radially from the center without any distinct spiral arm structures or prominent dust lanes visible. The core appears bright and moderately resolved, indicating a likely bulge component or a possibly weak active galactic nucleus. The overall color is slightly reddish, implying a stellar population that is relatively old and dominated by evolved stars, with potentially low levels of ongoing star formation. There might be a smaller companion galaxy with similar characteristics.

