The galaxy presents a predominantly smooth morphology, suggesting an elliptical or lenticular type. The central region exhibits a bright, concentrated core, indicative of a high stellar density and potentially a supermassive black hole. The overall color appears yellowish-red, implying an older stellar population with a lower proportion of young, blue stars. There is little evidence of distinct spiral arms or prominent dust lanes. A slight asymmetry can be observed in the galaxy's outer regions; this may be indicative of a past minor merger event. Overall the galaxy appears to be well defined and stable, with a clear center, and appears to have evolved significantly.
