The galaxy presents a predominantly smooth morphology, with evidence of a central bulge that is almost circular. The color suggests a mixture of stellar populations, with a brighter, possibly younger, population near the center exhibiting a bluish-green hue and older, more evolved stars indicated by the yellowish color toward the top. There appears to be a possible tidal arm or disturbed feature extending upward. This is a fairly compact galaxy, lacking distinct spiral arms or a well-defined disk structure. There is a possibility of an ongoing or recent minor merger event which would explain the slightly irregular appearance.
