The observed galaxy presents as an elongated, cigar-shaped structure, exhibiting a smooth, relatively featureless morphology. The primary light emission appears concentrated towards the central region, suggesting a prominent bulge or core. The color gradient transitions from a yellowish-orange core to a bluer, more diffuse outer region, hinting at potential variations in stellar populations or dust content. The apparent lack of distinct spiral arms or strong star-forming regions supports the classification of this galaxy as potentially an elliptical or lenticular type. There is a potential for tidal interactions or minor disturbances, although not clearly apparent at this resolution.
