The galaxy presents as a generally smooth, elliptical morphology. The color gradient transitions from a bright, yellowish core to a fainter, redder halo, indicating a likely older stellar population. There is a subtle suggestion of a flattened disk-like structure, but without distinct spiral arms or prominent dust lanes, it appears to be more spheroidally dominated. The galaxy does not show obvious signs of major merging or tidal disturbances, although a slight asymmetry cannot be ruled out. The light profile suggests that the galaxy is relatively relaxed, and well-defined.
