The galaxy presents as a lenticular or early-type spiral morphology, appearing relatively smooth with a discernible bulge. The galaxy exhibits a flattened, disk-like structure, although spiral arms are not distinctly visible in this image. The central bulge appears bright and concentrated, suggesting an older stellar population. There is evidence of a faint blue halo surrounding the central region. Overall, the galaxy appears to be in a relatively quiescent state of star formation. There are hints of tidal features, with the galaxy appearing slightly disturbed or warped. There appears to be at least one significant merging event occurring.
