The galaxy presents an elongated, somewhat irregular morphology, appearing as an edge-on or highly inclined disk. The light distribution suggests a central bulge region, although it is not distinctly pronounced, with a more diffuse and elongated structure. The galaxy shows a bluish hue, indicating the presence of a population of relatively young, hot stars. The observed colors suggest ongoing or recent star formation, particularly in the fainter regions of the galactic disk. The galaxy’s axial ratio appears to be approximately 0.35-0.45, revealing its flattened shape. The image does not clearly show prominent spiral arms, but there may be faint hints of spiral structure. The surface brightness appears relatively uniform across the galaxy, with only slight variations indicating density fluctuations in stellar populations. There is no evidence of strong tidal features, major mergers or significant disturbances to the overall structure. Overall, the galaxy appears to be a relatively undisturbed system, but the image resolution limits the ability to detect any fine details of its structure.