The galaxy appears as a single, relatively smooth object, exhibiting a concentrated central bulge that graduates into a less defined surrounding disk or halo. The galaxy presents a color gradient, with the central region displaying a yellow-orange hue. This suggests a potential concentration of older stellar populations and/or dust obscuration. The outer regions exhibit a bluer tint, possibly indicating the presence of younger, hotter stars within the galactic arms or disk. There are some slight, irregular features in the outer disk, suggestive of minor gravitational disturbances or active star formation regions. The general shape appears somewhere between round and elliptical, without any pronounced spiral arm structure easily apparent. No clear signs of an ongoing major merger are visibly evident, though some minor tidal features cannot be ruled out.
