This galaxy appears to be a spiral galaxy, observed nearly edge-on. The central bulge exhibits a concentrated, yellowish-white luminosity, suggesting an older stellar population. Extending outward from the bulge is a faint, flattened disk. This disk structure is visible due to its elongated shape. There is no visible evidence of a prominent dust lane. The disk shows only faint blue regions, indicative of ongoing or recent star formation. There is no obvious active galactic nuclei. There are no signs of significant tidal disturbances or ongoing major mergers. However, some minor asymmetry in the disk shape is observed. The overall morphology suggests this galaxy may be undergoing some type of interaction.