The galaxy presents as a somewhat elongated, cigar-shaped morphology. There is a distinct color gradient visible, shifting from bluer hues concentrated towards one end of the galactic structure to redder, more yellow tones at the opposite end. The region displaying bluer tones seems to indicate ongoing star formation activity. The redder end might suggest an older stellar population or dust obscuration. A slight asymmetry is apparent, with the bluer region appearing somewhat more prominent and less uniform than the more diffuse, redder section. The galaxy appears relatively isolated with only minor signs of interaction. 
