The galaxy presents as a single, centrally concentrated object. It is largely smooth in appearance, with no obvious spiral arm structures or significant dust lanes visible. The overall shape is close to circular. Color gradients suggest a higher concentration of older stars in the central region, with a slight blueing towards the outer edges. The light profile is fairly even, which is suggestive of an elliptical galaxy, although a highly inclined disk galaxy cannot be ruled out. There is little evidence of ongoing star formation or recent merger activity. The galaxy appears relatively undisturbed.
