The galaxy appears as an elongated structure, exhibiting a primarily smooth texture throughout its visible components. There is a slight concentration of light towards the central region, but this is not highly pronounced. A hint of a disk-like structure is present, contributing to the elongated shape. The color profile suggests ongoing star formation, primarily in the blue wavelengths, which are visible on the outer edges of the object. There is a noticeable asymmetry to the galaxy, potentially indicative of minor gravitational interactions or disturbances. Overall the galaxy exhibits characteristics intermediate between a fully formed elliptical and a spiral galaxy. It could be a disk galaxy viewed edge-on. There is evidence that mergers may be involved in the morphology of this galaxy.
