The galaxy presents as a spiral type, exhibiting a dominant central bulge and a distinct disk. The disk shows evidence of arm structure, although they appear somewhat flocculent. The bulge has a smooth, concentrated appearance. The galaxy is inclined relative to our line of sight, allowing a view of its disk. The color distribution indicates a mix of stellar populations, with bluer regions that are likely the locations of ongoing star formation. There is a slight asymmetry to the disk, potentially indicating past or ongoing interactions. The galaxy shows some signs of minor disturbance, potentially influenced by past or ongoing interactions, although it is not currently undergoing a major merging event.
