The observed galaxy exhibits a disk-like morphology, viewed at an oblique angle. Spiral arm structures are discernible, though somewhat flocculent in nature. These arms appear to originate near a central bulge which is neither overly prominent nor negligible. The central region exhibits a yellowish hue, potentially indicating a population of older stars. The disk shows blue regions, likely due to recent star formation. There is no strong evidence of a prominent bar structure within the galaxy. The disk appears largely undisturbed, lacking strong indications of ongoing major merger activity.
