The galaxy presents as a centrally concentrated, luminous object with a moderately elliptical morphology. The core exhibits a strong yellow-orange color, indicating a dominant population of older stars, likely within a bulge component. The light gradually diffuses outwards from the core, forming a halo with a less pronounced reddish hue. The halo appears smooth with no prominent spiral arm structures or significant dust lane features are readily apparent. The overall structure implies a relatively evolved system, possibly a lenticular or early-type spiral galaxy viewed at a large distance. Faint, subtle irregularities are suspected to exist. There is a hint of possible minor galactic interaction on one side of the galaxy.
