The galaxy presents as a relatively smooth, centrally concentrated object. The overall shape is somewhat elliptical, appearing mostly rounded in projection. There is no strong evidence of spiral arm structure or a prominent disk.

The galaxy exhibits a color gradient, appearing bluer towards the outer regions and redder in the central core. This color gradient may suggest a population of younger, hotter stars in the outskirts, and older, cooler stars concentrated in the center. However, dust obscuration may also be responsible for the color differences.

There are no obvious signs of major disturbances or ongoing merging events in this image. However, the possibility of minor tidal interactions with nearby galaxies cannot be ruled out based solely on this image. The galaxy's smooth appearance indicates that it is likely a relatively relaxed system.
