The galaxy presents as a single, relatively smooth concentration of light. The morphology is generally elliptical, displaying a shape that is neither perfectly round nor highly elongated. There's a central, brighter region that appears yellowish, suggesting an older stellar population. Fainter, diffuse light extends outwards from the core in a fairly regular manner, creating a soft, hazy halo. There is no obvious evidence of spiral arms or a prominent disk structure, nor are there any visible signs of a major merger or strong tidal disturbances. The color gradient suggests ongoing, though likely subdued, star formation activity, primarily in the galactic core.
