The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a moderately inclined disk with a prominent central bulge. The disk shows a smooth light distribution. The bulge is bright, concentrated, and elliptical in shape. There is no clear evidence of spiral arm structure or dust lanes within the disk. The galaxy has a moderate axis ratio. Color gradients are present, with the bulge appearing slightly redder compared to the disk. The galaxy appears relatively isolated, without any obvious signs of tidal interactions or nearby companions.
