The galaxy presents a flattened, elliptical morphology. The light distribution is concentrated towards the center, suggesting a dense core. The color profile exhibits a central region that is more yellow than its outer regions, which suggests an aging stellar population. The galaxy displays only subtle structures, showing a primarily smooth profile. There is little evidence of active star formation regions or significant dust lanes. Based on its apparent shape, the object is likely viewed at a significant inclination. There are no obvious signs of major merger events, although subtle irregularities might point to some tidal disturbance or minor interaction with smaller companion galaxies.
