The galaxy presents a generally smooth morphology. The primary light distribution suggests an elliptical or lenticular classification, with minimal evidence of spiral arms or distinct disk-like structures. The light appears centrally concentrated with a gradual decrease in intensity outwards, with a fairly regular, though not perfectly circular, shape. There is a slight color gradient observed, appearing bluer in the very central region, and shifting towards redder tones in the outer regions. There is no indication of a major ongoing merger, or tidal disturbances, such as tails. Any internal features are subtle and could be consistent with dust lanes or minor irregularities in the stellar population distribution.
