The galaxy presents as a somewhat elongated, disk-like structure. Its color profile suggests a more passive stellar population, exhibiting redder hues. The galaxy appears largely smooth, with minimal evidence of pronounced spiral arms or active star-forming regions. The light is concentrated towards the center. The disk exhibits some warping. There is some slight evidence of possible tidal features, but these are quite subtle and could also be artifacts of the imaging process. There does not seem to be much ongoing star formation.
