The galaxy presents as an elliptical system, exhibiting a smooth, largely featureless morphology. The core displays a higher concentration of light, suggesting a significant population of older stars or the presence of an active galactic nucleus. Moving outward from the core, the light gradually diffuses into the surrounding halo. There is evidence of a tidal tail on one side of the galaxy, suggesting past or ongoing gravitational interaction with another galaxy, or perhaps a merger event. The color is bluer in the center, indicating potential star formation, and then redshifts outwards. Overall, the galaxy's light profile suggests a mature system with a possible history of interaction.
