The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. A prominent bulge is visible, exhibiting a reddish hue, potentially indicative of an older stellar population. The outer regions display a more diffuse, bluish color, suggestive of the presence of younger, hotter stars. There is no apparent spiral arm structure or dust lane obscuration. The overall light distribution is relatively even and symmetrical, with a high degree of central concentration, indicating a relaxed system. There is no obvious evidence of recent major merger activity or tidal disruption. Minor irregularities and disturbances are not readily visible in the image. The galaxy appears to be a relatively undisturbed system with a dominant spheroidal component.
