The galaxy presents as a relatively smooth, centrally concentrated structure. It appears to be elliptical in shape, exhibiting a gradual decline in surface brightness from the core outwards. The core region shows a yellowish-white hue, suggesting an older stellar population. There is a subtle blueish tint to the outer regions which could possibly indicate the presence of some younger stars. There is no evidence of spiral arms or a prominent disk. There is no apparent interaction or obvious merging activity. Overall, the galaxy appears to be relatively isolated.
