The galaxy presents as a spiral galaxy with a prominent central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population, while the disk appears bluer, possibly indicating ongoing star formation. The spiral arms are tightly wound, exhibiting a moderate degree of structure. The galaxy appears to be inclined with respect to our line of sight, with an axis ratio indicating it is close to, but not quite edge-on. There is no obvious central bar feature. There is no clear evidence of a major merger or significant tidal disturbance. The galaxy seems to be fairly symmetrical and undisturbed.
