The galaxy presents as a somewhat elongated, likely disk-shaped structure. The central region exhibits a concentrated luminosity, indicating a prominent bulge. The overall color profile suggests a higher concentration of older stellar populations within the bulge, trending towards redder wavelengths. Fainter, bluer emissions are observed in the surrounding disk, hinting at regions of ongoing or recent star formation. The morphology suggests a relatively undisturbed system, though a slight asymmetry might indicate a minor gravitational interaction or internal dynamics affecting the structure. The galaxy's light distribution appears relatively smooth, with no prominent spiral arms or irregular features immediately apparent in this image. Further analysis is required to fully determine the galaxy's detailed morphology and star formation history.
