The galaxy exhibits a generally elliptical morphology. Its core appears bright and concentrated, with a yellowish-white hue suggesting an older stellar population dominating this region. The light emitted from the galaxy appears to be relatively smooth and symmetrical, indicating a lack of significant recent merger activity or major disturbances. 

A more diffuse, fainter halo surrounds the central region. The halo is not perfectly circular, but it is roughly elliptical. It is not possible to ascertain any complex structures such as spiral arms or dust lanes within the galaxy.

In terms of colour, there is a shift from the yellowish-white core to a slightly bluer outer halo, suggesting the presence of a younger, though still quite old, stellar population. The galaxy's overall appearance suggests that the galaxy is undergoing a low amount of star formation.