The galaxy presents as a centrally concentrated, smooth object. Its overall morphology appears elliptical, exhibiting a high degree of roundness. There is no apparent spiral arm structure or distinct disk component visible in this image. The galaxy’s light profile suggests a relatively homogenous stellar population, with no strong evidence of significant recent star formation activity. The primary colour is slightly yellow/gold in hue, suggesting an older stellar population. There are no signs of major mergers or tidal disturbances. Some minor asymmetry in the galaxy's light distribution might indicate a possible past interaction. The size appears relatively compact.
