The galaxy exhibits a generally elliptical morphology, though some structural asymmetry is apparent. It appears to be a relatively luminous object, with significant extent. There is a bright central bulge, which suggests an older stellar population, surrounded by a less defined disk-like component. Faint blue tinges within the outer regions, indicating a moderate level of on-going star formation within the galactic structure. There is a suggestion of tidal disturbances. Overall, the galaxy appears to be in some form of interaction or disturbance, indicating a potential recent or ongoing merging event.
