The galaxy presents a morphology consistent with a spiral type, although the arms are not particularly well-defined. The central bulge is prominent, exhibiting a concentrated, yellowish hue, indicative of an older stellar population. The disk component surrounding the bulge appears somewhat flocculent, with subtle indications of spiral structure, and there is not much evidence of current star formation. The galaxy is not viewed edge-on. There is no evidence of tidal tails or obvious signs of a major merger event.
