The galaxy presents a primarily elliptical morphology, exhibiting a smooth, concentrated central bulge that dominates its structure. The light distribution suggests a relatively uniform stellar population within the bulge, with a color profile that indicates the presence of older, redder stars. Fainter, bluer light is observable outside of the center, suggesting lower levels of current star formation. The overall galaxy structure does not display any significant signs of active merging or tidal disturbances. There may be faint disk-like features, but they're not well-defined in the image, obscuring the galactic plane.
