The galaxy appears as a centrally concentrated, smooth object, exhibiting a primarily elliptical morphology. The luminosity distribution is brightest in the core, gradually decreasing outwards. There is a subtle bluing of the light toward the center of the galaxy. The galaxy exhibits a slight degree of asymmetry in its outer isophotes, possibly suggestive of a minor interaction or past merger event. Overall, the galaxy presents a well-defined, somewhat rounded form without any prominent spiral arm structures or significant dust lane features.
