The galaxy presents as an elliptical or lenticular-type object. Its morphology is largely smooth and featureless, lacking any distinct spiral arms or prominent dust lanes. The light profile appears centrally concentrated, exhibiting a relatively high degree of overall symmetry. The color gradient suggests a population of older stars. There is no visible evidence of ongoing or recent major mergers. The light suggests the shape of this galaxy is in between round and cigar-shaped, leaning towards round. There seems to be little to no merging activity, but there may be a minor disturbance in the morphology of the galaxy.
