The galaxy presents a somewhat edge-on disk morphology, indicating a high inclination angle relative to our line of sight. A bright central bulge is visible, exhibiting a yellowish hue, suggesting an older stellar population in that region. The disk itself appears elongated and relatively thin, displaying a subtle color gradient, with a shift towards bluer tones in the outer regions. This may indicate ongoing star formation within the disk's spiral arms. There is a structure above the disk, but it is difficult to discern the exact nature of the feature. There may be a faint tidal tail or a disrupted companion galaxy. Additional observations would be required to confirm. Overall, the galaxy presents a clear disk-like structure, with a prominent bulge and evidence for both old and young stellar populations.
