The galaxy presents as a single, centrally concentrated object with a smooth morphology. The color profile exhibits a general yellowish-orange hue, suggesting a population of older stars. There is no discernible spiral structure, bar, or significant dust lane. The object appears highly spheroidal, with no apparent tidal features or signs of recent major merger activity. Faint, diffuse light extends outwards from the central region, fading into the background sky. Overall, the galaxy seems consistent with an elliptical classification.
