The galaxy presents a relatively smooth, elliptical morphology. It exhibits a high degree of central concentration with a noticeable decrease in luminosity as one moves radially outward from the core. The galaxy appears nearly round, showing minimal ellipticity. There is no clear evidence of spiral arms or significant disk structure. The galaxy's color profile indicates a population of older stars, with a generally redder hue. There may be low levels of star formation. There are no signs of major ongoing mergers or tidal disturbances.
