The galaxy presents as a spiral, viewed at a slight angle relative to face-on. The central bulge is moderately prominent and exhibits a yellowish-white hue, suggesting a population of older stars. Spiral arms are clearly visible, predominantly displaying a blueish color indicative of ongoing star formation. The arms appear relatively tightly wound around the bulge. There is evidence of a bar-like structure bisecting the central bulge, possibly extending into the inner spiral arms. The galaxy appears to be relatively isolated, showing no obvious signs of significant tidal interaction or major merging events with nearby galaxies, although there is a slight distortion visible in one of the arms. The disk is resolved, and there is a notable presence of star forming regions. The galaxy displays a clear spiral pattern.
