The galaxy presents a distinctly elongated, cigar-shaped morphology. Its overall color is a warm, yellow-orange hue, suggesting a stellar population dominated by older, less massive stars. The galaxy's light is smoothly distributed, with no apparent spiral arm structure or prominent dust lanes. This suggests a relatively uniform stellar distribution. There is a slight color gradient observed from the center, becoming slightly redder toward the outer edges, which could indicate ongoing, albeit subdued, star formation in the outskirts or simply a change in the composition of the stellar population. There is no visual evidence of recent major merger activity. The galaxy appears quiescent and relatively undisturbed, lacking any tidal tails or strong asymmetries.
