The observed galaxy presents as a moderately bright, disk-shaped structure, appearing somewhat flattened and elongated. The central region exhibits a higher surface brightness, suggesting a concentrated nucleus. Faint, diffuse extensions emanate from the central bulge, possibly indicating spiral arm structures, although these are not well-defined. The overall color profile suggests a mix of stellar populations, with bluer hues concentrated in the inner regions and a shift towards redder tones in the outer parts, potentially indicative of older stellar populations in the galactic halo. There is evidence of a minor tidal disturbance or interaction, potentially a smaller galaxy merging. The edges appear undefined.