The galaxy presents as a somewhat elliptical structure with a smooth overall appearance. There is a concentration of light towards the center, suggesting a possible bulge component. The color profile indicates a mixture of stellar populations, with a hint of bluer regions possibly indicating some ongoing star formation. The galaxy shows little evidence of strong spiral arm structure or significant morphological disturbances. Its shape tends toward being somewhat in between round and elliptical with a slight preference for elliptical. The galaxy does not present any strong signs of recent major merger activity.
