The galaxy presents as a slightly elongated, disk-like structure. Its central bulge appears prominent and exhibits a yellowish-orange hue, suggesting a population of older stars. The disk component appears less defined, showing some evidence of spiral arm structure, although this is faint. The arms are bluer in color than the bulge, implying a population of younger, hotter stars and potentially ongoing star formation. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal distortions. There's a subtle blue-ish hue in some areas of the disk region, possibly indicating regions of active star formation. The galaxy seems to be fairly smooth in appearance, with a slight bulge in the center.
