The galaxy presents a generally smooth morphology. The light distribution appears centrally concentrated, with a gradual decrease in brightness moving outwards from the core. The overall shape is predominantly rounded, with a slight elongation visible. There is a faint hint of a disk-like structure, though not sharply defined. No prominent spiral arms or bar features are discernible. The color profile suggests an older stellar population, possibly a relatively quiescent galaxy with a low rate of ongoing star formation, although the presence of some blue tinges hint to some ongoing starformation. There are no signs of any major mergers or significant tidal disturbances, only a few minor disturbances that could point to interactions.
