The galaxy presents a flattened, elongated morphology, reminiscent of a highly inclined disk system. The central region exhibits a higher surface brightness, appearing relatively smooth and featureless, suggesting a concentration of older stellar populations. Progressing outward from the core, the luminosity gradually decreases. The disk appears moderately blue, potentially indicative of recent or ongoing star formation, though this is not definitively discernible from the image alone. There is a subtle color gradient across the galaxy, trending towards redder hues in the central bulge and a bluer color as it moves away from the center. A faint and diffuse halo may be present, extending beyond the main disk. A hint of structural asymmetry can be seen, possibly indicative of past or ongoing interaction, or internal dynamics affecting the galactic structure.
