The galaxy appears to be a luminous, relatively compact object with a concentrated central bulge. It exhibits a primarily smooth morphology, with a slight hint of a disk structure or faint spiral arms. The color profile suggests a presence of older stellar populations, indicated by the reddish-yellow hue of the core and the overall golden appearance. There may be ongoing interactions or past merger events, indicated by the irregular shape, which could be interpreted as tidal features or disturbed morphology. Evidence of moderate star formation activity may be present, evidenced by the slight blue tinge on the edge of the object.
