The galaxy presents an elliptical morphology, exhibiting a smooth and relatively featureless structure. The light distribution suggests a high degree of central concentration, with a bright, nearly circular core. The overall color appears yellowish-orange, potentially indicative of an older stellar population, with a lower rate of on-going star formation. There appears to be minimal evidence of spiral arms, prominent dust lanes, or any signs of recent or ongoing major mergers, the outer regions appear slightly disturbed. The galaxy is roughly spherical, but not perfectly so.
