The galaxy presents as a relatively smooth, elliptical or lenticular structure. It displays a concentrated central bulge region, which appears bright and yellowish in color. This suggests an older stellar population dominates the core. Moving outwards from the core, the galaxy fades into a more diffuse halo. There is minimal evidence of spiral arm structures, active star formation regions or dust lanes visible in the image. The galaxy appears fairly isolated, with no obvious signs of tidal interactions or ongoing mergers. The overall color profile suggests a evolved system with low recent star formation activity, with the possibility of a very small amount of ongoing star formation. The galaxy appears compact. Overall, the system is well-defined and symmetrical in its morphology.
