The galaxy appears to be an elliptical type. Its overall shape is elongated, with a high degree of ellipticity. The central bulge exhibits a yellowish hue, suggesting an older stellar population with a lower rate of star formation, potentially composed of Population II stars. A disk component is possibly present, exhibiting a bluer coloration at the edges. This could indicate ongoing star formation in that region with younger, bluer Population I stars. There are no distinct spiral arms, but the overall shape may be slightly disturbed, potentially hinting at a past or ongoing minor merger event. The galaxy appears relatively smooth in overall texture and structure. 
