The galaxy presents a generally smooth, rounded morphology with a concentrated central bulge. A subtle disk-like structure may exist, though it is not sharply defined. The color profile exhibits a yellowish hue toward the center, likely indicating an older stellar population. Moving outward from the center, the color shifts towards a slightly bluer tone, suggesting the presence of younger stars or regions of ongoing star formation within the galaxy's periphery. No strong spiral arms or distinct dust lanes are apparent. There may be a very faint tidal tail present, but it could also be noise. Overall, the galaxy appears relatively undisturbed, with no obvious signs of a major ongoing merger, although minor disturbances can't be ruled out.
