The galaxy presents as a relatively smooth, consolidated light source. Its morphology is likely elliptical or lenticular, showing a minimal disk-like structure. The light profile is concentrated toward the center with a gradual decrease in surface brightness outwards. There's also some suggestion that the galaxy may be interacting, possibly in the late stages of a merger, or experiencing some minor tidal disturbance based on the presence of a separate and smaller clump nearby. The galaxy is exhibiting colours associated with an older stellar population suggesting low star formation rates. Overall, this galaxy is an example of an evolved system, with smooth, non-disk morphology.
