The galaxy appears to be a relatively smooth, elliptical-like object. It exhibits a concentrated central bulge region that appears bright white. Fainter, diffuse bluer emissions extend outward from the core, suggesting a more extended halo or disk component, although any distinct spiral arm structure is not apparent. The galaxy displays an approximately circular morphology, but also has the possibility of being mildly spheroidal. Overall, the galaxy presents a fairly regular and symmetric appearance, showing only minor signs of disturbance or recent mergers. Given its moderate size and brightness, this galaxy is likely a mid-mass system.
