The galaxy presents as a centrally concentrated, relatively smooth object with a slight ellipticity. The core exhibits a bright, yellowish hue, possibly indicative of an older stellar population. The outer regions display a subtle decrease in surface brightness, with hints of a transition towards redder colors, further supporting the presence of aging stars. There is a general lack of distinct spiral arm structures or prominent dust lanes. The overall morphology suggests an elliptical galaxy or a lenticular galaxy viewed at a shallow angle.
