The galaxy presents an elliptical morphology, with a smooth, diffuse light profile. The central region exhibits a brighter, more concentrated luminosity, gradually decreasing towards the outer edges. The overall color appears slightly blue, which is typical of galaxies with ongoing star formation, although this appears to be at a low rate. There are no distinct spiral arms or a prominent disk structure visible. There is a slight indication of some form of disturbance present in the galaxy. No significant tidal tails or other signs of major mergers are apparent, but minor disturbances can not be ruled out. The galaxy appears to be relatively isolated, showing no signs of strong interaction with nearby companions in the immediate field of view.
