The galaxy presents as a centrally concentrated spheroid, displaying a smooth, diffuse light distribution. The core exhibits a bright, concentrated glow, suggesting a high stellar density or potentially an active galactic nucleus, though this is not definitively discernible from the image alone. Moving outward from the center, the luminosity gradually diminishes, forming an elliptical halo. The shape appears mostly in between round and cigar shaped. Coloration is subtle, with a slightly blue hue in the outer regions that might indicate areas of more recent star formation compared to the yellowish-white core, which would indicate an older stellar population. There are no prominent spiral arms or distinct dust lanes visible. There is no evidence of a major merger or significant tidal disturbance affecting the morphology.
