The galaxy presents as a single, somewhat amorphous luminous structure. It exhibits a concentrated central region that transitions smoothly to a less dense outer halo. The overall color is yellowish orange, suggesting a population of older stars. The light distribution indicates that the galaxy is relatively smooth, lacking distinct spiral arms or a well-defined disk. The morphology suggests an elliptical or lenticular classification. The galaxy appears to be in the process of merging. A distinct double nucleus, possibly indicative of a major merger, is visible within the central region. The galaxy appears largely undisturbed aside from the ongoing merger, displaying no strong tidal tails or other signs of significant recent interaction.