This galaxy presents as a relatively edge-on spiral or lenticular galaxy. A central bulge is visible, appearing more concentrated and yellowish in color, potentially indicating an older stellar population. A flattened disk extends outward from the bulge. The disk exhibits a bluer hue than the central bulge, implying the presence of younger, hotter stars and ongoing star formation. The disk appears somewhat disturbed or uneven, possibly due to internal dynamics or interactions with a satellite galaxy. The overall structure suggests a galaxy of considerable mass, with an observable rate of star formation. There is no obvious active galactic nuclei, or AGN.
