The galaxy presents a primarily smooth morphology, with an apparent lack of spiral arm structures or distinct dust lanes. The light profile suggests a concentration of luminosity towards the galactic center. The overall shape appears to be somewhere between round and elliptical. There is a subtle indication of possible minor disturbances in the galaxy's structure, potentially related to tidal interactions or internal processes. The galaxy exhibits a redder color towards its core, possibly indicating an older stellar population or dust obscuration, with slightly bluer regions on the edges. The red and green color suggests that the galaxy is still forming stars but not at a fast rate. There also appears to be a possible galaxy merger in progress, with a companion galaxy close by and visible signs of possible streams of stars connecting the two galaxies. 
