The galaxy presents as a spiral galaxy with prominent, well-defined arms. The spiral arms are observed to have a tightly wound morphology. The central bulge of the galaxy is moderately sized and appears bright, suggesting a significant population of older stars. A faint bar structure may be present but is not strongly defined. The galaxy appears relatively isolated, with no major signs of recent or ongoing merging activity, although there is a slight irregularity in the arm structure that may indicate a minor interaction. Star formation appears active throughout the disk, as suggested by the blue hue observed in the spiral arms. The disk is viewed at a slight angle.
