The galaxy presents as a relatively smooth, disk-like structure with an elliptical morphology. The color profile indicates a dominant population of older stars, exhibiting a reddish-yellow hue overall. There is a slight indication of a central bulge, but it is not highly pronounced. The lack of clearly defined spiral arms or prominent dust lanes suggests a relatively quiescent star formation rate. The overall appearance points towards a galaxy that is in transition. There are no signs of any major merging events. 
