This galaxy presents as a somewhat inclined spiral, although with a structure that appears more bulge-dominated than a grand design spiral. The central bulge exhibits a yellow-orange hue, suggesting a population of older, cooler stars. Moving outward from the bulge, the disk is bluer in color, indicating younger, hotter stars and ongoing star formation. The spiral arms are not well-defined, appearing somewhat flocculent, but they are still visible nonetheless. There is no evidence of any major mergers, but the disk appears to be slightly disturbed, suggesting a possible minor interaction or past accretion event. The overall appearance indicates a galaxy of substantial mass and moderate star formation activity, with a significant fraction of its stellar population residing in a well-established bulge.
