The galaxy presents an elliptical morphology with a smooth, diffuse light distribution. There is a bright central region which gradually fades out towards the edges, suggesting a relatively concentrated stellar population. The lack of distinct spiral arms or a prominent disk structure further supports its classification as an elliptical galaxy. The overall color appears to be slightly blueish, perhaps indicating a moderate amount of ongoing star formation, although the smoothness suggests that the galaxy has likely been forming stars for a long time. There appears to be some minor asymmetry and perhaps some interaction with a neighbouring galaxy. The galaxy has been detected via HI measurements, confirming the presence of cool, neutral hydrogen gas and recent star formation.
