The galaxy presents an elongated, somewhat irregular morphology. A bright, centrally concentrated region dominates the galaxy's structure, possibly indicating a significant bulge or nucleus. Fainter extensions of light emanate from this central region, forming a disk-like structure. The disk exhibits a mottled appearance, suggesting some degree of inhomogeneity in its stellar populations or dust distribution. There is a possible indication of some tidal distortion or interaction given some of the wispy shapes in the light extending from the disk. Overall, the galaxy appears relatively compact, lacking prominent spiral arms or other clear features. The object appears to be faint, based on the color rendering of the image. Further analysis, including spectroscopic data, would be necessary to ascertain the galaxy's redshift, stellar content, and overall evolutionary state.
