The galaxy exhibits a somewhat elongated, cigar-shaped morphology. It appears largely smooth with a relatively featureless disk. There is a central bulge that contributes significantly to the overall luminosity. The color profile is generally uniform across the galaxy. The light from the central bulge appears more concentrated, fading towards the outer regions of the disk. There is a hint of some minor disturbances in the disk structure, although it lacks evidence of ongoing major merger activity. Star formation may be present, however it is not pronounced. 
