The galaxy presents as a smooth, centrally concentrated object with an elliptical morphology. Its core exhibits a bright, yellowish-white luminosity, suggesting a concentration of older stellar populations. The surrounding regions display a gradual decrease in surface brightness and a shift towards slightly redder hues. The isophotes are elongated, with a noticeable flattening. There is no evident spiral structure or dust lane features. The galaxy appears relatively undisturbed, without signs of major mergers or tidal interactions. The smooth light distribution and colors are consistent with an evolved galaxy dominated by older stars.
