This galaxy presents as an edge-on spiral, with a notable dust lane bisecting its length. The central bulge appears rounded and prominent, indicating a significant concentration of older stars in this region. Faint disk structures are observable, implying an ongoing level of star formation. There are no indications of significant morphological disturbance or signs of a recent major merger event in the galaxy’s structure. Based on its color indices, this galaxy displays a range of stellar populations. The galaxy exhibits a relatively high degree of inclination, with the disk appearing nearly perpendicular to our line of sight.
