The galaxy appears as a relatively smooth, centrally concentrated object with a diffuse, extended halo. Its morphology is largely spheroidal with only a hint of a disk-like structure. The color gradient suggests the presence of an older stellar population, particularly within the core, which exhibits a more yellowish hue. There may be a faint, elongated structure extending away from the core. There are no obvious signs of spiral arms or prominent dust lanes. Based on the galaxy's overall appearance, it appears to be a relatively massive galaxy with a low current star formation rate. There do not seem to be any major disturbances or merger activity affecting the galaxy's structure.
