The galaxy presents a predominantly smooth morphology, suggesting a classification as an elliptical or lenticular galaxy. Its overall shape is somewhat round. There is very little discernible substructure within the galaxy's light profile, with no clear spiral arms, dust lanes, or other prominent features typically associated with disk galaxies. The central region is characterized by a concentrated, bright core, surrounded by a more diffuse halo of light. The color is on the redder side which suggests an older stellar population and a low rate of on going star formation. There appears to be no significant signs of tidal disturbances or ongoing merger activity.
