This galaxy presents as a relatively compact and luminous object. It appears to be disk-shaped, viewed at a moderate inclination. The central region exhibits a brighter, yellowish hue suggesting an older stellar population. The outer regions of the disk display a distinctly bluer color, indicating the presence of ongoing star formation. This is further supported by the clumpy structures, possibly indicative of star-forming regions, within the disk. There is some visual evidence of minor disturbances present with a possible merging event present. The overall morphology could be described as a spiral or lenticular galaxy experiencing some interaction.
