The galaxy appears as a relatively compact, centrally concentrated object. Its overall shape is somewhat elongated, exhibiting an axis ratio that suggests a deviation from perfect sphericity. The light distribution is generally smooth, with a higher concentration towards the center, though some subtle variations can be observed. These variations may indicate some subtle features, such as spiral arms or dust lanes, but the resolution is not sufficient to confirm them.

The color of the galaxy appears slightly reddish, hinting at a population of older stars or the presence of dust that is absorbing blue light. The lack of distinct blue regions suggests a relatively low rate of ongoing star formation. There is no apparent significant interaction or merger activity ongoing with any other galaxy. It presents a relatively undisturbed morphology.
