The galaxy presents as a roughly elliptical object with a bright, concentrated central region. The core exhibits a saturated, white-blue color, suggesting intense star formation or potentially an active galactic nucleus. The outer regions display a fainter, diffuse halo with a greenish-blue hue, possibly indicative of a mix of older stellar populations and ongoing star formation. There are subtle hints of asymmetry or minor disturbances in the outer halo, though the overall structure appears relatively undisturbed. No prominent spiral arms or bars are discernible. The galaxy appears to be isolated, with no obvious signs of major merging activity or tidal interactions with nearby galaxies. The color profile, transitioning from white-blue at the center to greenish-blue in the outskirts, suggests radial variations in stellar populations and star formation rates.
