The galaxy presents as a slightly elongated spheroid, indicating an elliptical morphology, possibly of type E4 to E6. Its color is predominantly yellowish-orange toward the core, suggesting an older stellar population dominated by red giant stars. There is a subtle color gradient toward the outer regions, showing a slight bluish tinge hinting at the presence of younger, hotter stars in those areas, even though most of the star formation has ceased. The galaxy does not exhibit any spiral arm structures, bars, or prominent dust lanes. The light distribution appears relatively smooth and symmetrical, with no clear signs of active galactic nuclei, major tidal disturbances, or recent mergers. The light is concentrated to the center with gradually dimmer edges. Overall, the galaxy exhibits characteristics of a evolved system, having a substantial stellar mass and a relatively low star formation rate.
