The galaxy presents a generally smooth and centralized morphology. There is a concentrated central bulge exhibiting a yellow-orange hue, suggesting an older stellar population. The overall shape appears mostly round, showing minimal elongation. A faint, diffuse halo extends outwards from the central region, gradually fading into the background. There is no apparent spiral structure or significant dust lanes visible. No strong tidal features or signs of ongoing merger activity are readily apparent, suggesting a relatively undisturbed system. The galaxy is likely an elliptical galaxy based on its appearance.
