The galaxy presents an elongated, cigar-shaped morphology. Its central region exhibits a high surface brightness with a yellowish hue, suggesting an older stellar population or dust obscuration. The light gradually decreases toward the outer edges of the galaxy. A faint, extended halo is visible, displaying a blueish color. The galaxy appears relatively smooth, with minimal evidence of spiral arm structures or significant dust lanes. There is no obvious indication of a major ongoing merger, though subtle distortions may be present. Overall, the galaxy's appearance is consistent with that of a massive elliptical galaxy with a degree of star formation.
