The galaxy appears as a flattened, somewhat elongated object. The light distribution suggests a central bulge or core region with a higher concentration of older stars, exhibiting a yellowish hue. Extending outward from this core is a fainter disk component. While not clearly resolved, there is an indication of possible spiral arm structure, or at least some asymmetry within the disk. There seems to be a higher rate of star formation occuring in certain areas, these areas also have the youngest stars in the galaxy. No evidence of a close companion or recent major merger is apparent in the immediate vicinity. Overall, the object presents characteristics of a galaxy undergoing intermediate evolution.
