The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. Its overall shape is mostly round. There is little to no evidence of spiral arm structures or significant dust lanes. The galaxy's color profile suggests a relatively older stellar population, with a yellow-greenish central hue that fades into a darker, blue-ish halo. There is no indication of active merging or major disturbances in its morphology. The galaxy exhibits no strong evidence of ongoing star formation, consistent with a population of aging stars.
