The galaxy presents a prominent, moderately sized bulge region that appears yellowish in color, indicating a likely older stellar population. Fainter spiral arms emanate from this central region. These arms exhibit a bluer hue, indicative of younger stars and ongoing star formation, as well as evidence of dust lanes. The disk of the galaxy is viewed nearly face-on. There are no obvious signs of major interactions or mergers. However, subtle irregularities are visible, suggesting a possible minor disturbance or interaction history.
