The galaxy presents as a central, roughly circular bulge exhibiting a yellow-orange hue, indicative of an older stellar population. This core region is surrounded by a fainter, more diffuse disk. There is a subtle hint of spiral structure, though it is not well-defined. The disk appears relatively smooth, with only minor features, which indicates the presence of some star forming activity. The galaxy's overall light distribution suggests a moderate size, with an estimated absolute magnitude that hints at considerable luminosity. The light from the galaxy is redshifted, suggesting it is significantly distant from us. Overall, the galaxy appears to be largely undisturbed, showing no obvious signs of ongoing major merger events.