The observed galaxy appears to be a relatively compact system with a smooth, elliptical morphology. There is a central, bright core that exhibits high luminosity, gradually decreasing towards the outer edges. The galaxy presents with a moderate degree of roundness, with only slight deviations from a perfectly circular shape. There is no distinct disk-like structure visible, nor are there any obvious signs of spiral arms or active star formation regions. There appear to be no major disturbances or merging features evident in the image, suggesting a dynamically relaxed system. The galaxy exhibits an overall redder color, typical for older stellar populations.
