The galaxy presents as a moderately luminous, lenticular or elliptical system, appearing largely smooth and featureless in this image. It exhibits a central bulge that is elongated, suggesting a non-spherical structure. The luminosity appears to diminish gradually from the core outwards, indicating a relatively even distribution of stars within the galaxy's halo. Subtle color variations can be observed, the central core appears more yellow and the colors shift more blue/green in the outer edges, potentially representing distinct stellar populations or differing ages of stars present. There are no apparent signs of active star formation or significant dust lanes visible in the image. The overall morphology suggests a relatively quiescent galaxy that is past its peak of star formation. There is no clear evidence of spiral arm structures or signs of interaction with other galaxies.
