The galaxy presents as a spiral type, with a notable disk structure viewed at a slight angle relative to face-on. Two prominent spiral arms emanate from the central region, exhibiting a grand design morphology with loosely wound structures. Within the spiral arms, there appear to be localized regions of increased luminosity, suggesting ongoing star formation activity. The central bulge is moderate in size compared to the overall galactic disk. There is an indication of a bar-like structure extending through the galactic center. The galaxy displays no apparent signs of major interactions or recent mergers, although there may be minor irregularities in the outer disk. The galaxy possesses a color profile that suggests a mix of stellar populations across the disk, with bluer hues concentrated within the spiral arms and a generally yellower color towards the central bulge.
