The galaxy presents as a flattened, ellipsoidal form, consistent with a disk galaxy viewed at a high inclination. The central bulge appears prominent and exhibits a yellowish-orange hue, suggesting an older stellar population with fewer ongoing star formation events in the nucleus. Moving outward from the core, the disk displays a somewhat fainter, redder color profile. There's a hint of unevenness in the disk's light distribution, potentially indicating subtle spiral arm structures or dust lane obscuration, though these features are not clearly defined. The overall morphology leans towards a more regular, undisturbed structure, with no obvious signs of major tidal interactions or ongoing mergers. The galaxy has a relatively smooth appearance, without bright, knotty star-forming regions.
