The galaxy presents an overall flattened, disk-like morphology, viewed at a fairly high inclination. A prominent central bulge is observed, exhibiting a yellowish-orange hue, suggesting a population of older stars. The disk is less defined, with an overall bluish color, likely indicating the presence of younger, hotter stars and ongoing star formation. There is a slight asymmetry to the disk, but no apparent spiral arm structure. The galaxy appears relatively isolated, without any obvious signs of a major merger or tidal interactions. It exhibits a relatively smooth appearance. The outskirts of the galaxy fade gradually into the background, with no distinct halo observed in the image.