The galaxy presents a disk-like morphology with a predominantly smooth appearance. There is some indication of disk features. The galaxy exhibits a noticeable central bulge. The light distribution suggests an oblate spheroid shape, leaning toward being in between an elliptical and spiral galaxy in shape. No significant interactions or merger events with neighboring galaxies are immediately apparent. There may be evidence of minor disturbances within the galactic structure. The galaxy possesses an intermediate mass. It presents a relatively low star formation rate. It has some distinct red and blue colors throughout, with the red concentrated at its center.
