The galaxy appears to be an elliptical galaxy, exhibiting a smooth, largely featureless morphology. Its overall shape is round, although with a hint of elongation. The central region presents a bright, concentrated core, indicative of a substantial stellar population. Moving outward from the core, the luminosity gradually decreases, transitioning to a fainter halo. There is no discernible spiral structure or evidence of active star formation regions. Faint blue rings surround the galaxy, suggesting a past merger event. No significant tidal disturbances or signs of interaction with neighboring galaxies are apparent.
