The galaxy appears as a single, relatively smooth object with a concentrated central bulge. It exhibits a largely elliptical morphology, appearing quite rounded. There is no clear evidence of spiral arms or a prominent disk structure. The galaxy possesses a uniform color profile suggesting an older stellar population and low levels of ongoing star formation. There may be a potential interaction or merging event occuring with a smaller nearby object, causing some minor morphological disturbance. The object is not highly disturbed and shows a high degree of smoothness, meaning if there is a merging event, it has been a long time ago. 
