The galaxy presents as a fairly smooth, elliptical-like object. Its overall color appears to be a yellow-orange hue, suggesting an older stellar population. There are no distinct spiral arm structures visible, further supporting the smooth morphology. The galaxy exhibits a centrally concentrated brightness profile, diminishing towards the outer edges, without any obvious signs of a recent or ongoing major merger event. There is some slight color variation, but it is unclear from this image whether this results from internal dynamics or differential dust extinction. The overall round appearance suggests that it is not viewed edge-on. There is a suggestion of only minor disturbances. Star formation appears to be low. 
