The galaxy presents an elliptical morphology, appearing relatively smooth and centrally concentrated. There is a slight elongation, though it appears mostly round. Color gradients suggest a redder core, likely indicative of an older stellar population, with bluer regions possibly tracing ongoing or recent star formation in the outer parts. There are some possible signs of minor disturbances, although it is challenging to discern their nature with certainty. The galaxy displays no obvious spiral arms or a well-defined disk. Overall, the galaxy appears to be a massive system with a substantial stellar mass, at an advanced stage of its evolution.
