The galaxy appears as a diffuse, somewhat amorphous structure. It exhibits a generally smooth morphology, although subtle features suggest the possibility of a weak disk component. The central region shows a moderate concentration of light, but no distinct nucleus is readily apparent. The color profile is relatively uniform across the galaxy, with a subtle shift towards redder hues in the core. There may be minor signs of disturbance such as tidal tails or asymmetry, indicating a potential recent or ongoing interaction. There is evidence for a low star formation rate. The galaxy's structure appears to be undergoing little to no merging. The image suggests a galaxy that may be undergoing a slow transition in its star formation activity.
