The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears to be a dominant feature. The color is predominantly yellowish-orange, which suggests an older stellar population. The galaxy displays a high degree of roundness, with no clear indication of spiral arms or a distinct disk. There is a slight elongation or asymmetry visible, but the overall shape is close to spherical. No signs of a major ongoing merger are readily apparent. The galaxy has a substantial mass. Its star formation rate is relatively low.
