The galaxy presents a largely smooth, elliptical morphology. The core appears bright and relatively well-defined, with a gradual decrease in luminosity extending outwards. Some evidence of a disk-like structure is observed at the lowest part of the galaxy, though this is not the dominant morphology. The light distribution suggests an older stellar population, primarily red and yellow, with minimal evidence of active star formation regions from what is observed. There might be some minor disturbances. Overall, this galaxy appears to be a fairly evolved system, with a considerable mass and limited recent star formation.
