The galaxy presents a generally elliptical morphology with a bright, concentrated central bulge. The bulge exhibits a predominantly blue-white color, suggesting the presence of a younger stellar population or active galactic nuclei activity. Surrounding the bulge is a fainter, more diffuse region exhibiting a slightly reddish tint. The outer regions of the galaxy appear somewhat disturbed, possibly indicating minor tidal interactions or ongoing accretion events. There is a non-negligible fraction of light which does not appear to be associated with the galaxy. It may be related to foreground or background artifacts. 
