The galaxy presents as a somewhat smooth, centrally concentrated object, suggesting characteristics of an elliptical or lenticular galaxy. The primary body of the galaxy exhibits a generally rounded morphology. There is a possible indication of a minor disturbance or tidal feature located on one side of the galaxy that could possibly indicate a merger, but further analysis is needed to see if it is an artifact. Based on color, it looks as if there are likely older stellar populations within this galaxy, but further spectral information is required to understand the age and composition of the stellar populations present. This galaxy is likely undergoing moderate star formation, further spectral analysis is required for accurate confirmation.
