The galaxy appears as a generally smooth, centrally concentrated object, exhibiting an overall elliptical morphology. The light distribution is dominated by a bright, yellowish core, suggesting an older stellar population. There is evidence of a slight extension or halo surrounding the main body, with a gradual decrease in brightness from the core outwards. A subtle blueish tint can be seen in the outer regions, potentially indicative of some ongoing, albeit weak, star formation. There are minor distortions in the shape with slight disturbances visible. There seems to be some evidence of possible interactions with another galaxy, though is seems to be a minor disturbance. 