The galaxy presents a somewhat elliptical morphology, appearing significantly longer than it is wide. The light distribution suggests a concentration of luminosity towards the central region, potentially indicative of a bulge. Faint blue colored regions are observed in the outer reaches, suggesting some ongoing star formation. There is no clear evidence of spiral arm structure or a well-defined disk. The galaxy does not display any obvious signs of a major ongoing merger, although some minor disturbances cannot be ruled out. The overall appearance suggests a galaxy in a transitional phase.
