The galaxy presents a somewhat elliptical morphology, appearing as an oblate spheroid. It is dominated by a smooth, centrally concentrated component that is yellowish-orange, indicative of an older stellar population. A small amount of blue light, suggestive of a younger stellar population, may be present in the galaxy, but it is relatively indistinct, implying that star formation is low. There is no obvious spiral structure or distinct features, and it presents minimal signs of tidal disruption or merging events.
