The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears primarily yellow in color, suggesting an older stellar population. The surrounding halo is less concentrated and appears slightly more greenish, perhaps indicating some ongoing, but low-level star formation. The overall shape is somewhat flattened, falling somewhere between round and elongated. There is no clear evidence of strong tidal disturbances or major mergers. The galaxy appears to be a relatively isolated system with no obvious signs of interaction with neighboring galaxies.
