The galaxy presents as a concentrated, elliptical structure with a smooth, luminous profile. The core exhibits a yellow-orange hue, suggesting a population of older stars. The galaxy shows a high degree of central concentration, with luminosity decreasing gradually from the core to the outer regions. No distinct spiral arm structure is visible. The overall morphology appears undisturbed, lacking signs of major mergers or significant tidal interactions. There is little evidence of ongoing star formation.
