The galaxy presents a spiral structure, though somewhat flocculent. Well defined spiral arms emanate from a bright, moderately sized central bulge. The bulge exhibits a yellowish color, likely indicating an older stellar population. The spiral arms display a bluer hue, suggesting ongoing star formation activity within them. While the arms are somewhat patchy, they extend a considerable distance from the central bulge before fading into the background sky. There are hints of a bar-like structure running through the central region of the bulge. The galaxy appears relatively undisturbed, showing no strong evidence of recent major mergers. There may be minor asymmetries present in the outer arms, possibly indicating a weaker gravitational interaction or some other disturbance, but it could simply be a feature of the spiral arm structure itself. Overall, this appears to be a moderately massive spiral galaxy with active, though not exceptionally vigorous, star formation.
