The galaxy presents as a relatively smooth, centrally concentrated object, appearing largely elliptical in shape. A slight elongation is visible, but the galaxy does not appear highly flattened. The core exhibits a distinct, bright nucleus. The color gradient suggests a possible population of older stars dominating the galaxy, with a subtle presence of some younger, bluer stars in the outer regions. There are no prominent spiral arms or a well-defined disk structure visible. There is no noticeable disturbance to the symmetry of the object.
