The object appears to be a galaxy with a bright, compact central region, likely a galactic nucleus. The core exhibits a bluish hue, suggestive of a population of younger, hotter stars or possible active galactic nucleus activity. Surrounding the central region is a fainter, more diffuse halo. This halo displays a subtle color gradient, transitioning from greenish-yellow closer to the core to more reddish hues at the outer edges. This color gradient suggests variations in stellar populations or dust content across the galaxy, with older, redder stars potentially dominating the outer regions. There is evidence of minor morphological disturbance, which could be indicative of a past or ongoing minor merger event.
