The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a dominant central bulge. It possesses a smooth, luminous profile, with a slight elongation suggesting a disk component viewed at an oblique angle. There is a subtle color gradient, with the central region appearing more yellow-orange, possibly indicating an older stellar population. The outer regions of the galaxy are fainter and less defined, with minimal evidence of spiral arms or active star formation. The overall morphology is generally undisturbed, with no clear signs of recent mergers or major interactions. A faint, diffuse halo might be present, but this is difficult to discern with certainty given the image quality. The galaxy's intermediate redshift suggests it is a relatively distant object.
