The galaxy presents a generally smooth morphology. The central region is a concentrated, luminous bulge, exhibiting a yellowish-white hue, indicative of an older stellar population. Fainter disk-like extensions are observed, though ill-defined. These extensions display hints of bluer tones along the periphery, possibly suggesting regions of more recent star formation within the galaxy. The overall shape appears more elliptical than circular. No strong spiral arm structures or bars are apparent. There are indications of minor disturbances within the galaxy.