This galaxy exhibits a generally smooth morphology, with a high degree of central concentration. The light distribution appears elliptical rather than spiral. There is a bright, yellowish core, which may indicate an older stellar population. Surrounding this core, there is a less concentrated, greenish halo of light that extends to a few kiloparsecs. The galaxy does not appear to display any signs of major disturbances or mergers. There is no clear dust lane or arm structure. The galaxy has an intermediate roundness. The estimated mass of the galaxy is approximately 10^10.8 solar masses. The estimated star formation rate is relatively low.
