The galaxy presents as a somewhat elliptical, disk-like structure. The central region exhibits a concentrated, bright yellowish-white hue, suggesting an older stellar population. The outer regions of the galaxy are less defined, with a gradual decrease in brightness moving outwards. The color shifts towards a slightly bluer tone in these areas, potentially indicating the presence of younger stars and ongoing star formation, but the light is dominated by an old stellar population. There are no signs of spiral arms, major disturbances, or a prominent central bar within this image, and it seems to be a relatively isolated galaxy. The morphology appears to be largely undisturbed.
