The galaxy presents a predominantly smooth, elliptical morphology. The central region exhibits a high surface brightness, appearing almost uniformly luminous and yellowish. A gradual decrease in luminosity extends outwards from the core, forming a diffuse halo. There is a faint suggestion of a disk-like structure, but no distinct spiral arms are discernible. The overall color appears slightly redder, indicating a likely population of older stars and reduced ongoing star formation activity. There is no evidence of significant tidal distortions or merging events.
