The galaxy presents as a singular object, with a smooth, centralized light distribution. The morphology appears elliptical rather than spiral, exhibiting a somewhat rounded shape. There's a subtle color gradient, with the core appearing slightly yellower than the outer regions. No distinct spiral arms or dust lanes are discernible. The overall texture of the galaxy is relatively uniform with only slight color variations, indicating a largely homogenous stellar population, suggestive of an older system with less ongoing star formation. There is no clear evidence of any major ongoing mergers or tidal disturbances affecting the system's overall structure.
