The galaxy appears as a diffuse, centrally concentrated object with a predominantly smooth morphology. The light profile exhibits a gradual decrease in intensity from the core outwards, suggesting a bulge-dominated system. There are some subtle color variations throughout the galaxy, but these are minimal. The galaxy shows a fairly even color distribution. There are also a few small irregular areas with light. There is no prominent disk or spiral structure apparent in the image. While the galaxy appears relatively undisturbed, there are some asymmetries in the outer regions that suggest a possible minor interaction or past merger event. There is no clear evidence of tidal tails or strong distortions. The overall impression is that of a fairly relaxed system, with minimal ongoing star formation activity.
