The galaxy presents as a slightly elongated, centrally concentrated object. Its color profile suggests a more evolved stellar population, with a yellowish-white core indicative of older stars. The galaxy appears relatively smooth in texture, lacking prominent spiral arms or distinct dust lanes. There is the possibility of some subtle disturbances in the overall structure but appears to be undergoing a possible minor merging. The is an indication of some ongoing star formation, with the outer edges having a blue tinge to them. It appears to be a massive galaxy with an elevated star formation rate.
