The galaxy presents as a centrally concentrated elliptical or lenticular morphology, exhibiting a smooth and relatively featureless structure. The light distribution suggests a spheroidal shape with a dominant bulge component. There's a color gradient, with the central region appearing slightly yellower, transitioning to bluer hues in the outer regions. The central region could indicate an older stellar population while the bluer light in the outer regions may suggest younger stellar populations. There's no apparent spiral arm structure. Marginal indications of minor asymmetries within the outer envelope, though these may arise from tidal interactions with neighboring galaxies or minor internal disturbances.
