The observed galaxy presents as a roughly elliptical, moderately compact object. Its core exhibits a bright, concentrated luminosity with a blue-white hue, suggestive of a significant population of young, hot stars or potentially an active galactic nucleus. Surrounding the core, there is a somewhat amorphous, greenish halo with faint, diffuse extensions. There are subtle hints of structural features like asymmetry or possible tidal distortions, implying potential interactions with other galaxies. Given the smooth appearance of the central region, it is unlikely to have strong spiral arms, but we note some faint features in the greenish halo that could be dust and gas associated with past interaction or star formation. More spectroscopic analysis would be required to confirm the nature of the inner nucleus.
