The galaxy presents as a somewhat disturbed spiral or lenticular system, viewed at a moderate inclination. The overall structure appears elongated, with a primary concentration of light toward the center that suggests the presence of a bulge. The system shows evidence of disruption and possible interaction. There are irregular extensions or tidal features extending away from the main body, more prominent on one side, indicating potential gravitational interactions or recent merger activity. Colors are primarily blue, concentrated in the tidal-arm-like features, which suggests ongoing star formation in those regions. A dust lane feature might be partially obscuring the central bulge. There are other features that are either dust or small pockets of star formation.
