The galaxy presents a largely smooth morphology. The light is concentrated towards the center with a bright central bulge. The central region exhibits a yellow-orange hue, indicating a possible population of older stars. There's a slight blue-green tint on the outer edges of the galaxy, potentially suggesting more recent, albeit mild, star formation in these regions. The galaxy appears to be relatively undisturbed with no obvious signs of a recent major merger, though there is a small nearby companion galaxy that could potentially lead to a minor disturbance later on. The shape is nearly circular, suggesting it is likely to be an elliptical galaxy. The radial luminosity profile decreases smoothly outwards from the core.
