The galaxy presents a largely smooth, elliptical morphology with a bright, concentrated central bulge. The overall color is a pale blue, suggesting the presence of a moderate population of younger, hotter stars, particularly in the inner regions. There is a subtle extension of the galaxy's light along a major axis, giving it a slightly elongated appearance, but it lacks a well-defined disk structure. There is some hint of disturbance to the galaxy's form, but nothing overtly suggests a major ongoing merger, though a minor interaction or past event can not be ruled out based on morphology alone. There appears to be little to no dust obscuration visible in this image.
