The galaxy presents as a somewhat elongated, lens-shaped structure. The central bulge exhibits a smooth, reddish-orange hue, indicative of an older stellar population. Fainter, greenish-blue patches are observed in the outer regions, suggesting pockets of more recent star formation. The overall morphology is relatively undisturbed, with no strong evidence of tidal tails or major merger events. The galaxy exhibits a significant axis ratio, appearing cigar shaped, potentially indicating it may be an elliptical galaxy. The presence of both smooth and featured components suggest it is not a simple elliptical but may have a disk. The observed color gradients imply variations in stellar populations across the galaxy.
