The galaxy presents as a relatively smooth, elliptical-like structure, with a bright, concentrated central bulge. The galaxy exhibits a color gradient, appearing more yellow/red toward the center and subtly bluer in the outer regions. This suggests a population of older stars concentrated within the bulge, while younger, bluer stars may exist in the surrounding disk or halo. There is a slight hint of a disk structure, but no prominent spiral arms are visible. A faint, diffuse halo extends outwards from the main body of the galaxy. There is a slight asymmetry in the galaxy's shape. A small distortion or possible minor merger event cannot be ruled out. There seems to be dust or an area of obscuration present slightly off from the center. Overall, it appears to be a moderately massive galaxy with ongoing, though potentially declining, star formation.
