This galaxy, at a redshift of approximately 0.31, exhibits a primarily smooth morphology. The central region appears concentrated, emitting strongly in g, r, and z bands, indicating a significant population of older stars. The galaxy's shape is generally round, with a hint of disk-like structure. There may be some disturbances within the galaxy, suggestive of minor gravitational interactions, though the overall form is not highly disturbed. While the central core shines yellow-orange, there are hints of redder areas. The galaxy's estimated size suggests it is a relatively large and massive system, likely in the later stages of its evolution, with low levels of current star formation.
