This galaxy exhibits a spiral morphology, presenting with a prominent disk. Two well-defined spiral arms are visible, extending from a central bulge region. These arms appear somewhat tightly wound. The central bulge is relatively moderate in size, contributing a substantial amount of light, although it is not overly dominant. The spiral arms show a range of stellar populations as traced by their color, with subtle variations in brightness that may indicate regions of active star formation. Overall, this galaxy does not show any obvious signs of major interaction or merging events.
