The galaxy presents as a distorted spiral with an apparent red shift. The core region is elliptical, displaying a smooth, diffuse light distribution, with a color suggesting an older stellar population. Emanating from this core are spiral arms, though the overall structure is somewhat disrupted, exhibiting signs of tidal interactions or a recent merger event.

One arm shows a more prominent star formation rate. The galaxy appears to be in a dynamic state with active regions of star formation. The mass is on the lower end compared to other galaxies, and it is estimated to have a low rate of star formation. The estimated size of the galaxy suggests it is a small to medium size.
