The galaxy presents as a relatively smooth, disk-like structure with a noticeable central bulge. It is elongated, exhibiting a cigar-like shape. The central region appears yellowish, suggesting an older stellar population. The outer regions of the disk display hints of bluer hues, possibly indicating ongoing star formation, though the rate appears to be low. The disk shows some evidence of subtle disturbance, it does not appear to be undergoing a major merger or violent interaction. The overall structure suggests a galaxy that is transitioning towards a more quiescent state.
