The galaxy presents a somewhat face-on orientation with a bright, concentrated central bulge. The bulge appears yellow-white, indicative of an older stellar population. Surrounding the bulge, a faint, extended disk is visible. The disk material has a mottled bluish hue, suggesting the presence of younger, hotter stars and ongoing star formation. Faint spiral arm structures can be discerned within the disk, though they are not sharply defined. Overall, the galaxy exhibits a smooth, elliptical-like appearance, with a central bulge. There is no apparent evidence of significant tidal interactions or merging activity.
