This galaxy exhibits a notably smooth morphology, with a high degree of central concentration. It is mostly round, lacking significant features indicative of a spiral or barred structure. There appears to be a lack of any prominent, dust lanes or intricate features, although, there seems to be a possibility of merging occurring. The light profile indicates an older stellar population, primarily emitting in the redder wavelengths. Overall, this galaxy appears to be an elliptical or lenticular galaxy, with a relatively high mass, experiencing limited star formation.
