The galaxy presents as a centrally concentrated elliptical, exhibiting a generally smooth morphology. Its shape appears somewhat flattened, resembling a rounded disc when viewed from our perspective. The central region displays a bright, concentrated luminosity, indicating a high density of stars or possibly an active galactic nucleus. The light gradually fades as one moves outward from the core, with a diffuse halo extending beyond the main body. No distinct spiral arms or significant dust lanes are readily apparent in this imaging. There appears to be a slight blue shift towards the outer edges. There is a hint of disturbances within the halo of the galaxy, perhaps indicating a past merger.
