The galaxy presents a generally smooth, elliptical morphology. It exhibits a bright, concentrated central bulge, surrounded by a fainter, more diffuse halo. The overall color appears slightly redder in the central region, suggesting an older stellar population, with the halo showing some blueish tint, indicating younger stars. There's a hint of a possible minor disturbance or asymmetry in the halo on the left side, which could indicate a past merger event or tidal interaction. The galaxy appears fairly isolated with no obvious major companions or signs of ongoing merger activity.
