The galaxy appears as a centrally concentrated, elliptical-type system. Its overall color is yellowish-orange, suggestive of an older stellar population, with perhaps lower rates of ongoing star formation. The morphology is smooth, exhibiting a high degree of radial symmetry and lacking prominent spiral arms or distinct structural features, but also suggesting a possible disk. It does not show strong signs of tidal disturbances or interactions with other galaxies, although there may be a very slight irregularity in its outer isophotes.
