The galaxy appears to be a relatively bright, lenticular or early-type spiral galaxy, seen at an oblique angle. The central bulge is prominent and exhibits a yellowish hue, suggesting an older stellar population. The disk surrounding the bulge presents a bluer tint, implying the presence of younger stars and ongoing or recent star formation. The galaxy is not perfectly symmetrical; there are some subtle irregularities in its outer regions, hinting at potential minor gravitational interactions. There is no clear evidence of a major ongoing merger. The object has an apparent size consistent with it being a relatively massive galaxy at a moderate redshift. The overall morphology indicates that it is undergoing a transition, possibly evolving from a more actively star-forming spiral toward a quiescent elliptical galaxy.
