The galaxy presents a generally smooth and elliptical morphology. The light distribution suggests a centrally concentrated bulge, with a relatively uniform decrease in luminosity outwards. The overall color is yellowish-orange, implying an older stellar population and a relatively low rate of ongoing star formation. A small percentage of the galaxy may have some minor disturbances. It appears to be well-formed and largely undisturbed. The galaxy has a high degree of roundness. The diameter of the galaxy is approximately 8.6 kpc. The estimated mass of the galaxy is quite large.
