The galaxy exhibits an elongated morphology, potentially indicating a disk-like structure viewed at an oblique angle. The light distribution is not uniform, suggesting some internal structure. A brighter, more concentrated region is visible near what appears to be the center of the galaxy, possibly a galactic bulge or nucleus. Faint, diffuse emission extends from this central region outwards, primarily towards one side, giving the appearance of a tail or extended arm. The color profile shows variations, with bluer hues concentrated in patches within the main body, indicative of possible star-forming regions. Some areas suggest a reddish tint, which could be due to older stellar populations or dust obscuration. There appears to be a slight warping or disturbance in the shape, especially in the extended arm or tail, suggesting possible tidal interactions or past mergers. Overall, the galaxy displays characteristics of a spiral or irregular system undergoing some form of dynamic process.
