The galaxy presents as a relatively smooth, elliptical form. A dominant central bulge appears bright and slightly elongated with a yellow-orange hue, suggesting an older stellar population. Fainter, disk-like extensions are observed along the major axis, displaying a bluer color gradient away from the core, potentially indicating younger stars and ongoing star formation. There's a subtle indication of some minor tidal disturbance, possibly the result of a minor merger in its past. The overall structure does not show any prominent spiral arms or strong signs of active merging.
