The galaxy presents a roughly elliptical morphology, though with some visible asymmetry. The central region exhibits a high surface brightness, appearing largely smooth and yellowish-white. The outer regions display a fainter, more diffuse structure with some hints of spiral arms. The overall color gradient suggests a potential decline in stellar population age from the center outwards. Some blue knots can be seen in the fainter regions, indicating areas of star formation. A slight warp or distortion in the galaxy's outer profile could be suggestive of a past or ongoing minor interaction. There appears to be some disturbance of the main galaxy shape. Overall, it appears to be an intermediate-mass galaxy with a moderate amount of star formation. 
