The galaxy presents a generally smooth, elliptical morphology. Its light profile exhibits a centrally concentrated bulge, fading into an extended, diffuse halo. The central region appears predominantly blue, suggesting ongoing or recent star formation, while the outer regions show a redder hue, potentially indicating an older stellar population. The galaxy displays a moderate level of roundness, showing only a slight elongation. There are no obvious signs of spiral arms or a prominent disk structure. There is a subtle, asymmetrical feature, possibly a minor disturbance in the galaxy's outer halo. Based on these observations, the galaxy can be classified as an elliptical galaxy experiencing some low-level star formation.
