The galaxy presents as a singular, concentrated body with a smooth, largely featureless morphology. Its overall shape is predominantly round, exhibiting minimal deviation from circular symmetry. A slight elongation may be present, but the galaxy appears generally spheroidal.

Color analysis reveals a dominant yellowish-white hue in the central region, suggestive of an older stellar population. The outer regions display a subtle shift towards redder tones, which could indicate a gradient in stellar age or composition.

There is tentative evidence of a possible minor disturbance or interaction; however, the dominant impression is that of a well-established system. There is no indication of a significant disk structure.
