The galaxy presents as a spiral galaxy observed nearly edge-on. A prominent central bulge is evident, exhibiting a smooth, concentrated morphology. The bulge appears reddish-yellow in color, possibly indicating an older stellar population and/or dust obscuration. A disk structure is clearly visible extending from the central bulge. The disk appears thin and elongated, oriented almost perfectly along our line of sight. There are some apparent clumpy regions within the disk, possibly indicative of star formation. No evidence of a major ongoing merger is apparent. However, subtle irregularities in the disk structure may suggest some tidal disturbance. Overall, the galaxy appears to be a relatively massive system undergoing moderate star formation.
