The galaxy presents as a luminous, centrally concentrated object with an apparent near-spherical morphology. Its core appears bright and somewhat yellow. There is a faint, diffuse halo extending outwards, primarily along one axis, giving it a slightly oblong appearance. The light distribution suggests a system dominated by an older stellar population, with relatively low ongoing star formation. There is a secondary, smaller object to one side, which appears to be interacting with the primary galaxy, but more data is needed to confirm. Given the mass and size, it is likely a large galaxy, the slight asymmetry could be a sign of a minor merger event.
