The galaxy presents as a disk galaxy, viewed nearly edge-on from our vantage point. There appears to be a significant central bulge component dominating the overall light profile. The bulge exhibits a smoothly distributed light, with a rounded morphology. The disk component is relatively thin and elongated, extending outwards from the central bulge. Light from the disk is less intense, showing signs of some obscuration likely by dust lanes within the plane of the galaxy. The galaxy exhibits an overall reddish-yellow hue. The galaxy does not appear to have any prominent spiral arm structures or evidence of a recent major merging event. There might be a minor disturbance within the disk, or possibly an asymmetrical distribution of light and dust.
