The galaxy presents a diffuse, somewhat amorphous structure. It appears to be composed of two distinct components. The primary component exhibits a centrally concentrated bulge, yellow in color, surrounded by a fainter, bluer halo. The overall shape of this component is irregular. A secondary component appears as a smaller, more elongated structure with a yellowish hue, possibly a spiral arm or a tidal tail. There is weak evidence of ongoing or recent interactions, given the disturbed morphology and potential tidal features. Star formation activity may be present in the bluer regions, but is not obviously vigorous.
