The galaxy appears as an elongated, disk-shaped structure. The central bulge is a bright, concentrated yellowish-orange hue, suggesting an older stellar population with a lower rate of star formation. The outer regions of the galaxy exhibit a bluer color, possibly indicating the presence of younger, hotter stars and regions of active star formation. There is a subtle gradient in color intensity from the center outwards, with the core appearing far brighter than the outer disk, indicating the increased concentration of stars toward the center. The galaxy exhibits a relatively smooth overall texture, with no clear signs of significant dust lanes or spiral arm structures visible at this resolution, suggesting that it is likely a relatively undisturbed galaxy. There are no clear signs of recent major mergers or tidal distortions.
