The galaxy presents as an elliptical morphology, appearing largely smooth in structure. Its light is centrally concentrated, displaying a radial decrease in surface brightness without prominent spiral arm features. The color profile indicates a population of older stars, likely with lower ongoing star formation. There is no distinct bulge or disk component observed, supporting its classification as an elliptical. The galaxy appears undisturbed, showing no signs of tidal tails or other morphological distortions indicative of recent mergers or interactions. It shows a generally round shape.
