The galaxy presents a predominantly smooth morphology, lacking distinct spiral arms or a pronounced disk structure. The light distribution appears centrally concentrated, exhibiting a diffuse, elliptical shape. The core of the galaxy displays a yellowish hue, potentially indicative of an older stellar population. The outer regions fade gradually, showing hints of a faint, redder halo. There is no immediately apparent evidence of ongoing major mergers or significant tidal disturbances. Overall, the galaxy's characteristics suggest an evolved system, possibly an elliptical galaxy or a lenticular galaxy viewed face-on, with a relatively quiescent star formation rate.
