The galaxy exhibits a morphology consistent with an elliptical or lenticular classification. It presents a smooth, centrally concentrated light profile. There is an apparent lack of prominent spiral arm structures or significant dust lanes. The overall shape is elongated, but moderately rounded, with an axis ratio suggesting it is viewed at a shallow angle. Color gradients suggest a slightly bluer outer halo region, which may indicate ongoing, but minimal, star formation activity in the outskirts. The central region is yellower, possibly indicative of an older stellar population. There may be some minor tidal disturbances, but overall it appears to be an isolated system.
