The galaxy presents as a generally smooth, elongated object. A bright, concentrated central bulge dominates the core region. It appears that the bulge is surrounded by a fainter, more diffuse disk component. The disk shows hints of structural features, but they are not well-defined. The overall color of the bulge appears slightly redder compared to the surrounding disk, suggesting an older stellar population in that area. There is no obvious indication of a major ongoing merger. The elongation of the galaxy suggests it is likely elliptical or a lenticular galaxy viewed at an angle.
