The galaxy presents as a somewhat elongated or cigar-shaped structure. The central region exhibits a higher concentration of light, appearing yellowish-white, potentially indicating an older stellar population. Fainter, bluer light emanates from the outer regions of the galaxy, possibly suggesting areas of more recent star formation. There are signs of some minor disturbances or asymmetries in the galaxy's structure. Based on the visible color gradient, it is likely a spiral galaxy viewed at an angle. 
