The galaxy presents as a disk galaxy, viewed nearly edge-on from our line of sight. There is a prominent central bulge, appearing yellowish-white in color. This suggests an older stellar population within the bulge. The disk surrounding the bulge shows hints of structure but lacks clear, well-defined spiral arms. The color of the disk is slightly bluer than the central bulge, indicating the presence of younger, hotter stars and potentially ongoing star formation. The disk appears somewhat asymmetric and slightly warped, with a faint, diffuse halo extending beyond the main disk structure. No significant signs of a major ongoing merger or strong tidal features are apparent. There appears to be a hint of a faint dust lane along the disk, further obscuring details of star formation within. Overall, the galaxy appears to be a relatively massive and luminous galaxy with a mix of stellar populations and some signs of recent or ongoing star formation.
