The galaxy presents as an elliptical morphology, with a smooth and relatively featureless appearance. Its shape appears somewhat elongated, exhibiting a cigar-like form rather than a perfectly round structure. There is a clear central bulge that gradually diffuses outwards. Color gradients are subtle, with a slightly more reddish hue concentrated towards the core, suggesting an older stellar population. The outer regions appear bluer. Overall, the galaxy displays a lack of any significant disk or spiral arm structures. There is no obvious indication of a major ongoing merger, although minor disturbances cannot be ruled out.
