The galaxy presents as a concentrated, elliptical-like form with a bright, prominent central bulge. The bulge exhibits a yellowish-orange hue, likely indicating an older stellar population. The surrounding disk appears less defined, with a smoother texture and a bluer tint in some regions, suggesting the presence of younger, hotter stars and some ongoing star formation. There is a slight asymmetry in the outer regions of the disk, hinting at potential interactions or minor disturbances, but no major merging events are immediately evident. Overall, the galaxy appears to be relatively massive, with suppressed star formation activity for its mass, residing at a redshift of approximately 0.138.
