The galaxy presents as a roughly elliptical object, exhibiting a relatively smooth morphology. There is an absence of strong spiral arm structures or a prominent central bar. The primary light distribution is concentrated centrally, suggesting a high degree of radial symmetry. The galaxy's color profile appears slightly redder when compared to other visible objects in this image. Faint asymmetries can be detected and may indicate the presence of minor disturbances due to a potential interaction with another galaxy. The light is spread out in this galaxy, not exhibiting any highly compact regions. Overall, it suggests a relatively evolved system, possibly transitioning towards a more quiescent state with a low rate of ongoing star formation.
