The galaxy presents as a lenticular or early-type spiral galaxy, exhibiting a primarily smooth, elliptical morphology. A bright, concentrated central bulge dominates the galaxy's structure. The surrounding disk is visible, though it appears relatively faint and featureless, lacking prominent spiral arm structures. The galaxy is elongated, with an apparent cigar shape, suggesting an inclination relative to our line of sight. There is no obvious evidence of recent major merger events or significant tidal disturbances, and a smooth halo of stars surrounds the structure. The lack of prominent star-forming regions suggests a low star formation rate within the galaxy.
