This galaxy appears to be a spiral galaxy, viewed at an oblique angle relative to our line of sight. The galaxy exhibits a central bulge that appears brighter and more concentrated. The disk of the galaxy is visible, showing a relatively smooth distribution of light, suggesting a relatively well-mixed stellar population. There is a subtle hint of spiral arm structure, which is relatively indistinct. The galaxy presents a reddish-yellow hue indicative of an older stellar population with reduced recent star formation. No significant dust lanes or prominent star-forming regions are readily apparent in the visible light. Based on its apparent smooth morphology, this galaxy has likely experienced a period of quiescence in terms of star formation activity. There is no evidence of a major merger.
