The galaxy presents as an elliptical, disk-like structure with a distinct central bulge. The bulge exhibits a concentrated luminosity gradient, appearing bright and yellowish-white. Moving outward from the central bulge, the light diffuses into a less concentrated, fainter disk. The disk's color shifts towards bluer hues as it extends away from the core, implying the presence of younger stellar populations in the outer regions. There is a slight suggestion of a spiral structure, or possible dust lanes within the galaxy, however this is hard to distinguish clearly. The galaxy appears generally smooth, with no major morphological disturbances or interactions evident in the image. It seems relatively isolated, with no obvious companion galaxies nearby. The galaxy is generally elongated, suggesting that it is not a face-on spiral galaxy, and has an inclination relative to our line of sight.
