The galaxy presents as a relatively smooth, elliptical morphology. There is a discernible central bulge which appears more yellow, possibly indicating an older stellar population and lower star formation rate in this region. The outer regions are less concentrated and appear slightly bluer, hinting at the presence of younger, hotter stars. The galaxy exhibits no obvious spiral arms, strong dust lanes, or signs of major mergers. There is perhaps a slight asymmetry, suggesting a past minor interaction or disturbance. The overall structure is generally round with a slightly elongated appearance.
