The galaxy presents as an elliptical morphology, exhibiting a concentrated central bulge with a smooth, diffuse halo. Its overall shape tends towards a somewhat flattened spheroid, appearing as a round but not perfectly circular object. The color profile suggests an older stellar population, indicated by a redder hue, with the highest concentration in the galactic nucleus. No prominent spiral arm structures or dust lanes are discernible. There may be some minor distortions in the halo, but they do not strongly suggest a major ongoing merger.
