The galaxy presents as a relatively smooth, centralized structure. Its overall shape appears to be somewhat elliptical but is difficult to fully discern, appearing between round and slightly elongated. The central region displays a bright, concentrated luminosity, suggesting a dense stellar population or possibly an active galactic nucleus. Moving outwards from the center, the luminosity gradually diminishes. There appears to be a hint of a disk. Its color is primarily yellowish-white at the core, transitioning to a subtle blueish hue in the outer regions. No prominent spiral arm structures are clearly visible, nor are any signs of major disturbances or ongoing merging events immediately apparent. There is a faint irregular structure in the outermost regions. The galaxy's features suggest a high probability of it being a relatively massive system.
