The galaxy presents as a disk galaxy observed nearly edge-on. There is a prominent central bulge, appearing yellowish, suggesting an older stellar population. The disk exhibits a relatively smooth texture, showing minimal distinct spiral arm structure. A faint dust lane appears to be present along the equatorial plane, obscuring some of the light from the bulge. The bulge appears to be slightly rounded and centrally concentrated. There is no evidence of major mergers or significant tidal disturbances. Based on the color profile, star formation rate appears relatively low.
