This galaxy presents as an elliptical or lenticular morphology, characterized by a predominantly smooth light distribution. Its overall shape appears largely spheroidal with slight elongation. There is no distinct spiral arm structure visible. The galaxy's color gradient suggests a higher concentration of older stellar populations towards the center. Faint bluer regions are present in the outer areas. There is no strong indication of active galactic nuclei or recent major merger activity, although subtle irregularities in the outer envelope might suggest minor gravitational interactions in its history.
