The galaxy presents as an edge-on spiral, with a prominent, elongated disk oriented nearly horizontally. There is a distinct central bulge that appears bright and concentrated, exhibiting a yellowish hue, potentially indicating a population of older stars. The disk is characterized by a color gradient, transitioning from a yellowish tone near the bulge to a bluer hue in the outer regions. This suggests active star formation in the outer disk, typical of spiral galaxies with ongoing gas and dust accretion. The dust lane bisecting the galaxy is subtle but observable. There appears to be some irregularity or minor disturbance within the disk, but there is no obvious, ongoing major merger. The bulge appears to be a mostly rounded shape. Overall, it appears to be a large galaxy undergoing active star formation, with an estimated mass that is very large. 
