The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. The light distribution appears relatively uniform, indicating a lack of significant spiral arms or distinct features. Color gradients suggest an older stellar population dominating the galaxy's composition. The overall rounded appearance of the galaxy signifies minimal distortion or ongoing merger activity. There's a slight elongation in its shape. Despite the overall smooth appearance, subtle hints of disturbances cannot be entirely ruled out, suggesting the possibility of minor gravitational interactions in its past.
