The galaxy presents as a centrally concentrated object, with a smooth and generally rounded morphology. The central region exhibits a yellowish hue, indicating a potential population of older stars or dust obscuration. There appears to be a lack of prominent spiral arm structures or a well-defined disk. Faint extensions, or perhaps minor tidal disturbances, might be present around the main body of the galaxy, though these features are not highly pronounced. The object displays an intermediate redshift, suggesting its light has been stretched by the expansion of the universe. While it appears relatively undisturbed, there are hints of minor gravitational interactions, such as slight asymmetry in the light distribution. Overall, it could be classified as an elliptical galaxy, possibly undergoing a minor merger event.
