The galaxy presents a largely smooth, elliptical morphology. It exhibits a high degree of central concentration with a bright, yellow-orange core, suggesting an older stellar population. Fainter greenish colors appear mottled around the central bulge. The disk or outer regions of the galaxy appear largely featureless in terms of spiral arms or distinct dust lanes. The overall light distribution suggests an evolved system with a low current star formation rate. There is no apparent interaction or merging event occurring based on the galaxy's shape and the lack of tidal tails or distorted structures. The galaxy appears relatively isolated in the field.
