The galaxy exhibits a generally elliptical morphology, appearing somewhat elongated in shape. A bright, concentrated central bulge dominates the structure, displaying a yellowish-white hue, indicative of an older stellar population. Surrounding the bulge is a fainter, more diffuse disk component. Within the disk, subtle hints of spiral structure can be discerned, although they are not sharply defined. There's a slight bluer tint to the outer regions of the disk, which may suggest more recent star formation activity. Overall, the galaxy's appearance suggests a transitionary state, possibly between a spiral and lenticular galaxy, with characteristics of both.
