The galaxy presents a largely smooth and centrally concentrated morphology. Its light profile appears to be relatively symmetrical, showing a gently decreasing luminosity gradient from its bright nucleus outwards. The shape of the galaxy is elliptical, appearing mostly rounded rather than elongated, and not particularly disk-like. The lack of any apparent spiral arm structure or significant dust lanes reinforces its classification as an elliptical galaxy. There is no visual evidence of any ongoing major mergers or significant tidal disturbances. There might be very minor signs of interaction, but it does not disrupt its overall smooth appearance. The galaxy's color suggests an older stellar population, consistent with an elliptical galaxy that has largely ceased active star formation.
