The galaxy presents a smooth, elliptical morphology. Its central bulge appears bright and concentrated, exhibiting a yellow-orange hue, suggesting an older stellar population dominated by red giants and supergiants. The galaxy lacks a clear spiral arm structure or prominent dust lanes. The outer regions gradually fade into the background, indicating a decreasing stellar density. The overall shape is somewhat elongated, displaying a moderate ellipticity, but it doesn't resemble a highly flattened disk. There is little evidence of ongoing star formation activity in the visible spectrum; the colors are generally consistent with a passively evolving system.
