This galaxy exhibits a notably elongated morphology, appearing cigar-shaped in its overall form. A distinct central bulge is visible, suggesting a concentration of older stellar populations. Extending from this central region is a fainter, more diffuse structure possibly consistent with a galactic disk viewed edge-on. There is evidence of asymmetry in the disk's extension, with a slightly brighter and more pronounced region appearing off-center. This asymmetry could potentially indicate an interaction with another galaxy, although no obvious tidal features are discernible. The galaxy's color is predominantly reddish, implying a population dominated by older, redder stars and potentially significant dust obscuration. Limited signs of ongoing star formation are evident from the overall color. A small, somewhat detached structure, possibly a dwarf galaxy or a star cluster, is visible near one end of the main galaxy body. Further analysis with higher resolution imaging and spectroscopic data would be beneficial to investigate the nature of this extended structure and to determine the galaxy's exact morphological type and any ongoing interactions.
