The galaxy presents as a somewhat amorphous, centrally concentrated object. It exhibits a bright, yellowish core that appears relatively smooth, possibly indicative of an older stellar population or significant dust obscuration. Fainter, bluish diffuse regions surround the core, suggesting the presence of younger stars and ongoing star formation. There is a faint disk-like structure that can be seen. There is some visual evidence of minor morphological disturbances. Based on the color distribution, the galaxy shows moderate star formation activity.