This galaxy appears to be a relatively compact object, exhibiting a flattened, disk-like morphology when viewed from our vantage point. The galaxy presents a general hue that transitions from a central bluish-white to a more diffuse, greenish-yellow surrounding the core. The central region shows strong luminosity suggesting a high concentration of stellar activity.

A distinct feature is the presence of a blue ring structure around the object, possibly indicative of active star formation within a rotating disk. Within this ring are features of red emission. These red features, in conjunction with the blue, possibly indicate ongoing star formation. The galaxy lacks any obvious spiral arm structure or significant dust lanes, indicating a possibly smooth stellar distribution, or is possibly an early stage spiral galaxy. The general form exhibits only minor disturbances suggesting a somewhat isolated system with no major ongoing mergers or interactions, though some features might suggest minor disturbances.
