The galaxy presents as a somewhat elongated structure, oriented approximately vertically within the image. It exhibits a smooth, centrally concentrated luminosity profile, suggesting a relatively evolved system. The color gradients indicate a predominantly older stellar population, particularly within the central region which appears more yellow and red-toned. Fainter blue hues along the outer edges suggest the presence of more recent, though limited, star formation. The overall shape implies a disk-like morphology but the galaxy is presented edge on, with evidence of significant flattening. There is some indication of minor disturbances in the disk.
