The galaxy presents a smooth, somewhat elongated profile, suggesting an elliptical morphology, though some disky features cannot be ruled out. The concentration of light is high towards the center, fading gradually outwards. The galaxy's color appears to be redder than average, indicating a population of older stars and a lower rate of ongoing star formation. There is no obvious evidence of a recent major merger or significant tidal disturbances, although the galaxy does show a mild elongation. Faint traces of possible minor interactions cannot be entirely excluded given the image resolution. The overall appearance is consistent with a massive, evolved system.
