The galaxy presents as a flattened, elongated structure, highly suggestive of a disk galaxy viewed edge-on or a prolate elliptical galaxy. Its morphology appears largely smooth and featureless, lacking prominent spiral arms or distinct clumps of star formation. The color profile exhibits a gradient, appearing more luminous and perhaps slightly bluer centrally, fading towards the outer regions with a shift towards redder hues. This could indicate a concentration of younger, hotter stars in the core, and older stellar populations dominating the outskirts. The overall symmetry and lack of obvious tidal features do not suggest a recent major merger event, although a minor disturbance cannot be entirely ruled out. The galaxy's apparent size is relatively small, implying either a physically compact object or a significant distance. Overall, the galaxy appears to be a relatively quiescent system, potentially with moderate levels of star formation confined to its central regions.
