The galaxy presents a relatively smooth, elliptical morphology. There is a distinct central bulge that appears yellowish-white in color, suggesting an older stellar population is dominant in this region. The galaxy appears elongated, exhibiting an axial ratio that is clearly non-spherical. The outer regions of the galaxy show a gradual decline in surface brightness. There is a slight hint of a disk-like structure, but no distinct spiral arms or significant dust lanes are visible. The color gradient transitions from the yellow-white core to a slightly bluer hue in the outer regions, possibly indicating the presence of some younger stars at the edge of the galaxy. There is no visual evidence of any major mergers or significant tidal disturbances in the galaxy's structure.
