The galaxy presents a diffuse, somewhat elongated morphology. The central region appears relatively smooth and concentrated, with a gradation towards less defined outer regions. Coloration is predominantly blue-shifted suggesting ongoing or recent star formation activity. There is indication of disturbance in the overall structure, a slight asymmetry is observed and the color is not uniformly distributed. A small, tightly condensed region exists that may be the result of minor galaxy interaction. There is no obvious spiral structure or prominent dust lanes.