The galaxy appears as a relatively smooth and concentrated object with a dominant central bulge. Its overall color profile suggests a higher concentration of older stellar populations. The light is dominated by redder wavelengths, transitioning to a yellow hue at the core. There is a distinct lack of obvious spiral arm structures or significant dust lanes. The shape appears mostly elliptical, with the object showing relatively little elongation. There seems to be no major morphological disturbance within the galaxy's immediate vicinity. The galaxy's structure suggests that it may be in a relatively quiescent state. Based on the image, its estimated size is relatively compact.
