The galaxy exhibits a generally elliptical morphology, presenting a relatively smooth appearance overall. It displays a prominent central bulge that dominates the galaxy's light profile, with a high concentration of light towards the core. The bulge exhibits a yellowish-white hue, suggesting an older stellar population. Surrounding the bulge is a fainter disk component. The disk shows evidence of bluer light indicative of younger stars and/or star forming regions. The disk also contains evidence of spiral structure, although they are not sharply defined. The galaxy is seen at an inclined angle. There may be minor disturbances of the symmetry. The overall structure suggests a galaxy somewhere along the lenticular or early spiral classification.
