The galaxy presents as an elliptical, exhibiting a smooth, largely featureless morphology. Its overall shape appears nearly circular. The central region displays a high concentration of light, suggesting a prominent galactic nucleus or bulge. The color profile indicates a mix of stellar populations, with the central bulge tending towards warmer hues, potentially indicative of older, redder stars. Surrounding the central bulge, there is a gradual transition to a slightly bluer, yet still subdued, halo. There is no evident spiral arm structure, bar, or distinct dust lane obscuring its form. The galaxy does not appear to be undergoing any major ongoing merger events, though there may be faint hints of minor disturbances in the outer halo.
