The galaxy exhibits an overall elliptical morphology, appearing somewhat elongated rather than perfectly spherical. The central region displays a concentrated luminosity, suggesting a significant density of stars or an active galactic nucleus. Moving outwards from the core, the light gradually diminishes.

There's a hint of a possible interaction or minor disturbance in the galaxy's structure, potentially indicated by subtle asymmetries or tidal features. The galaxy's color profile shows variations, with the core exhibiting a warmer, yellower hue, while the outer regions have a bluer tint. This color difference implies a potential variation in stellar populations or dust content, where the core may be populated by older, redder stars, and the outskirts may have younger, bluer stars.
