The galaxy appears to be a somewhat elongated structure, exhibiting a moderate degree of smoothness. There appears to be a slight distortion of the primary galactic disc with no clear spiral arm structures. It's major axis is oriented roughly horizontally in the frame. There is a subtle color gradient from a relatively bluer central region to redder outer parts of the galaxy suggesting ongoing star formation. This star formation might not be occurring at a high rate. The light profile indicates it is a galaxy with an approximate diameter close to 10 kpc. There is no evidence of a major merger event, although minor disturbances cannot be ruled out given the slight asymmetry.
