The galaxy exhibits an irregular morphology. A centrally located, somewhat diffuse, and moderately bright region appears as a dominant feature. The color of the central region presents as a slightly desaturated yellow.

There appears to be a fainter, elongated structure or plume extending away from the central region. The color in this plume appears bluer. This could indicate younger stellar populations within that area.

There is evidence of what could be further disturbances or faint features, possibly indicative of interactions or minor mergers. The overall visual impression suggests a system undergoing some form of evolutionary process or interaction.
