The galaxy presents as a centrally concentrated luminous object, exhibiting a primarily smooth morphology. There is a slight elongation or asymmetry suggesting it may be tending towards a spheroid or disk shape, as opposed to a perfect sphere. The core region displays a yellow-white hue, potentially indicating an older stellar population or a concentration of dust. The outer regions appear dimmer and bluer. While generally undisturbed, there's a hint of a minor perturbation in the morphology, possibly from a past or ongoing interaction with another galaxy.
