The galaxy presents a slightly elongated, disk-like morphology with an intermediate axial ratio. It appears to have a relatively smooth structure, although subtle features or faint arms may be present within the disk. The galaxy exhibits a blueish hue, suggesting the presence of a younger stellar population and ongoing star formation. Overall, it appears to be a relatively undisturbed galaxy, showing no major signs of merging or significant tidal interactions. The galaxy has a moderate effective radius, and is likely a spiral galaxy.
