The galaxy presents as a moderately luminous, lenticular or early-type spiral, galaxy. It appears elongated, with a high axial ratio, suggesting an edge-on or nearly edge-on orientation with respect to our line of sight. The central bulge appears dominant and exhibits a smooth, concentrated light profile, with a yellowish hue suggesting an older stellar population. Faint disc-like structures are visible extending outward from the bulge. The absence of well-defined spiral arms implies a relatively quiescent star formation rate. There are no indications of a major ongoing merger, however, the disk appears slightly disturbed on one end, suggesting possible minor gravitational interactions. The galaxy has a redshift of 0.173150, indicating a significant distance.