The galaxy appears as a centrally concentrated, somewhat rounded entity. Its light profile appears relatively smooth. There is no distinct spiral structure or bar visible. Color gradients are subtle, with a suggestion of bluer light emanating from the core. The outer regions are less distinct, suggesting a gradual decline in star formation rate towards the galaxy's periphery. The image suggests it is a fairly quiescent galaxy, with potential for ongoing but mild star formation in the central region. There is some indication of possible minor disturbances or tidal features.
