This galaxy appears to be a complex system, potentially undergoing interaction or exhibiting internal disturbances. The morphology is neither purely elliptical nor a well-defined spiral. A significant fraction of its light is concentrated in a relatively smooth, central region, suggesting the presence of an older stellar population. However, there also seem to be regions of bluer light, indicating the presence of younger stars and ongoing star formation. There are also hints of tidal features or asymmetries in the outer regions, though they are not pronounced. Overall, this galaxy appears to be of intermediate mass with a moderate amount of star formation.
