The galaxy presents an elliptical morphology, exhibiting a smooth and relatively featureless light distribution. The central region displays a concentrated, bright core, indicative of a high stellar density, possibly hosting a supermassive black hole. Moving outward from the core, the luminosity gradually decreases, forming a diffuse halo. There is minimal evidence of spiral arm structure or significant dust lanes. The overall color suggests a population of older stars with less active star formation present. The shape approximates an ellipse that is noticeably elongated. There are no signs of interaction with other galaxies.
