The galaxy presents as a lenticular or early-type spiral. The central bulge is prominent and exhibits a smooth, concentrated distribution of light, suggesting an older stellar population. A faint, extended disk surrounds the bulge, exhibiting a bluer color, hinting at possible ongoing or recent star formation. The disk appears elongated, indicating a flattened shape. Faint spiral arm structures may exist, but they are not well-defined in the available image. There appears to be a potential merger occurring with a small and amorphous galaxy nearby. The orientation of the galaxy is such that we view it at an inclined angle. Overall the galaxy is characterized by an intermediate luminosity.
