The galaxy appears to be a single, relatively smooth object. Its morphology suggests it is elliptical or lenticular, exhibiting a centrally concentrated light profile that fades gradually outwards. The shape is largely round, deviating only slightly from perfect circularity. There is a subtle color gradient, with the central region exhibiting a slightly yellower hue, potentially indicative of an older stellar population. Faint hints of bluer colors are present in the outer regions, possibly suggesting more recent star formation, although this is not distinct. There is no apparent evidence of spiral arms, a bar structure, or significant dust lanes. There appears to be very minor tidal disturbance, if any. Overall, the galaxy appears to be a mature system with a smooth light distribution and likely a high fraction of evolved stars.
