The galaxy presents as a centrally concentrated elliptical type with a smooth, diffuse morphology. It exhibits a roughly spherical shape, with a bright, well-defined core that gradually decreases in luminosity towards the outer regions. The color profile suggests a population of older stars, indicated by a yellowish-red hue in the central region. There are very faint blue tinges in the outskirts of the galaxy. There is no evidence of spiral arms, a prominent disk, or significant dust lanes. There are no obvious signs of recent or ongoing major merger events.
