This galaxy presents a relatively compact, disk-like morphology with a slightly elongated shape. The central region exhibits a bright, concentrated luminosity, potentially indicating a high density of stars or an active galactic nucleus. A subtle color gradient is observed, with the core appearing bluer and the outer regions trending towards redder hues. This suggests differing stellar populations, with younger, hotter stars dominating the core and older, cooler stars populating the outskirts. Faint, diffuse extensions are visible emanating from the central region, possibly indicative of a galactic halo. No prominent spiral arms or significant dust lanes are immediately apparent, leading to an overall assessment of a galaxy lacking strong, well-defined features. Minor disturbances may be present.
