The galaxy appears as a relatively small, disk-shaped structure. Its central region exhibits a bright, concentrated light, suggesting the presence of a dense stellar population or active galactic nucleus. Faint spiral arm-like features are suspected, although the disk's overall structure is not clearly defined. The galaxy's color profile indicates a possible mix of stellar populations, as the central region appears more blue than other surrounding regions. No obvious signs of significant tidal interactions or major disturbances are observed.
