The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. There is a dominant bulge component, characterized by a yellowish-white hue, suggesting an older stellar population. A faint, diffuse halo surrounds the central region, gradually fading into the background. There is no apparent structure indicative of spiral arms or a prominent disk. The galaxy does not show any obvious signs of recent major merger activity, though subtle tidal features may be present upon further analysis.
