The galaxy presents as a moderately luminous, elliptical-like structure. It exhibits a smooth, featureless morphology with no discernible spiral arms or bar. The light distribution suggests a concentrated central bulge that fades into a diffuse halo. The galaxy's shape is elongated, appearing cigar-shaped. There is a color gradient visible, with the central region displaying a yellowish-orange hue, indicative of an older stellar population, while the outer regions appear slightly bluer. The overall appearance suggests a galaxy with a substantial mass and a relatively low rate of current star formation. There is no indication of any ongoing merger activity or major tidal disturbances.
