The galaxy presents as a centrally concentrated object with a smooth, spheroidal morphology. The light distribution is dominated by a bright, compact core, indicating a significant concentration of stars. The outer regions of the galaxy fade gradually, showing no evidence of spiral arms or a distinct disk component. There may be slight signs of distortion and merging activity. It exhibits a blue-shifted hue, suggesting relatively recent star formation. The galaxy appears relatively isolated, without any nearby companions or tidal features.
