The galaxy presents as a largely elliptical morphology with a smooth, concentrated central bulge. There are no apparent spiral arm structures discernible in this image. The galaxy's core exhibits a yellowish-orange hue, possibly indicative of an older stellar population, while the outer regions appear bluer, hinting at the presence of younger, hotter stars. The overall appearance is relatively undisturbed, lacking significant tidal features or signs of ongoing major mergers. There may be some minor asymmetries or irregularities in the outer halo, but these are not distinct. The galaxy appears to be relatively isolated.
