The galaxy presents an overall elliptical morphology. There is a central bulge with a relatively smooth appearance. The apparent shape is elongated, with the major axis significantly longer than the minor axis.

Faint, diffuse light is visible extending outwards from the central bulge. This indicates a more extended halo or disk component, however the faintness of the feature makes it difficult to discern any distinct structures. The overall color of the galaxy appears to be approximately uniform, suggesting a consistent stellar population or dust distribution throughout the visible region.

There is no strong evidence of spiral arms or prominent dust lanes. There are hints of minor disturbances in the shape of the outer halo. No other obvious signs of ongoing mergers are present within this image.
