The galaxy presents a generally smooth and rounded morphology. There is a noticeable concentration of light towards the galactic center, suggesting a prominent bulge. Fainter, diffuse light extends outwards, indicating a relatively faint disk, assuming the galaxy has one. There is a slight asymmetry in the outer regions, but this is not indicative of any major disturbance or ongoing merger. The overall color is slightly red-shifted, indicating an older stellar population, with low star formation. It's a fairly isolated object, and the morphology is consistent with an elliptical or S0 type galaxy.
