The galaxy presents as a smooth, elliptical-like object with a centrally concentrated bulge. It is generally lenticular or elliptical in form, appearing flattened along its major axis with a notable absence of spiral arm structures. The galaxy exhibits a yellow-reddish hue, particularly in the central region. This suggests an older stellar population and potentially lower levels of ongoing star formation. The outer regions appear fainter and bluer, possibly indicating the presence of younger stars. The overall morphology suggests a relatively evolved system, where star formation has largely subsided, and the constituent stars are aging. There is no clear evidence of any significant mergers or tidal disturbances affecting the morphology of the galaxy.
