The galaxy presents a notable central bulge region with a concentrated, bright, yellowish hue. Emanating from this central region is a slightly elongated and diffuse disk structure, appearing somewhat mottled in texture. The overall color profile suggests a mix of stellar populations, with the yellowish core hinting at older, redder stars, and the fainter blueish component in the disk region indicating regions of active star formation. Some asymmetries or disturbances are present, especially near the central regions, possibly pointing to past or ongoing interactions. The shape is between a disk and a more spheroid shape, with a slight roundness overall. Possible signs of merger activity are visible, with some slight disturbances and asymmetry. 
