The galaxy presents as a spiral, exhibiting a pronounced disk structure viewed at a slight incline. The spiral arms are well-defined and appear flocculent in nature, with numerous regions of active star formation indicated by a bluish hue. A central bulge is visible, exhibiting a moderate size relative to the overall disk. The core of the bulge appears bright and concentrated. A bar feature is present, though not particularly dominant. There are indications of tidal disturbances, possibly suggestive of an interaction or past merger event, though no major morphological disruption is evident. The galaxy displays a redshift indicating significant distance, implying substantial luminosity despite its apparent size. Its color suggests ongoing star formation with a mass within a reasonable range for galaxies of its type.
