The galaxy presents a flattened, elongated morphology, suggestive of a disk galaxy viewed at a significant inclination. The central region exhibits a brighter, more concentrated luminosity, possibly indicating the presence of a galactic bulge. The overall color appears to be yellowish, which may be indicative of an older stellar population. There are very faint blue areas that are potentially areas of star formation. No obvious spiral arm structure is discernible within the image, potentially due to the high inclination or smoothing of the image. The galaxy appears relatively undisturbed, with no obvious signs of major merger activity or tidal distortions. The structure is primarily smooth.
