The galaxy presents a somewhat elongated, cigar-shaped morphology. The central region exhibits a concentrated, yellowish-orange hue, suggesting an older stellar population or significant dust obscuration. Moving outwards from the center, a diffuse, greenish-blue disk is observed. The overall color profile indicates ongoing star formation, though primarily concentrated away from the galactic nucleus. No major tidal features or evidence of recent major mergers are apparent. The galaxy appears relatively undisturbed, possibly undergoing minor interactions. The disk appears somewhat clumpy, suggesting localized regions of higher star formation activity. The galaxy is moderately luminous. 
