The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, relatively featureless morphology. The light distribution appears concentrated towards the center, with a gradual decrease in intensity outwards. The overall shape is elongated, resembling a cigar shape. There is no evidence of spiral arms or distinct disk features visible. The color profile suggests an older stellar population, possibly dominated by redder stars and a limited amount of on-going star formation. No signs of major mergers or significant tidal disturbances are observed, although a slight asymmetry could indicate a minor interaction in its past.
