The galaxy presents as a relatively smooth, centralized object with a near-spherical morphology. There's little evidence of distinct spiral arms or a pronounced disk structure. The light distribution appears centrally concentrated, with a gradual fading towards the outer edges. The core region exhibits a brighter, more intense luminosity, suggesting a concentration of stars or possible active galactic nucleus activity. There might be slight color variations, but overall, the color is somewhat uniform. There are no apparent signs of ongoing major merger activity or significant tidal disturbances, and the image suggests an isolated system, without clear interactions with nearby galaxies.
