The galaxy presents as a centrally concentrated, luminous object. The core region exhibits a bright, relatively smooth, and concentrated appearance in the g-band, suggesting a significant population of older stars. Moving outward from the core, there's a gradual decrease in luminosity. The overall shape appears largely elliptical, with a high degree of roundness, although there may be some minor asymmetry or disturbance visible in the outer regions. There is some evidence of ongoing star formation as indicated by redder coloration. It is possible that this galaxy is undergoing a minor interaction or merger event given the disturbance noted.
