The galaxy appears to be a relatively smooth, elliptical type. It presents a concentrated central bulge. The galaxy exhibits a generally round morphology with some slight deviation. There is minimal evidence of spiral arms or disk-like structures. Faint, diffuse outer regions surround the core, suggesting a gradual decrease in stellar density with increasing distance from the galactic center. There is no strong evidence of a major ongoing merger event; any disturbances are either minor or not readily apparent at this resolution. The overall color is indicative of an older stellar population.
