The galaxy presents as a smooth, elongated structure. It exhibits a clear central bulge, brightest in the image, transitioning into a less concentrated disk. The color profile suggests a relatively evolved stellar population, leaning towards older, redder stars. The disk is subtly bluer in some areas, suggesting regions of ongoing, but diminished, star formation. The galaxy is moderately inclined with a cigar shape. There is no evidence of active galactic nuclei or major disturbances, though faint tidal features cannot be definitively ruled out given the image quality.
