This galaxy presents as a flattened elliptical, or possibly a highly inclined spiral galaxy with tightly wound arms. The central bulge appears prominent and exhibits a yellowish hue, suggesting an older stellar population. The disk component, if present, is viewed edge-on, contributing to the galaxy's elongated shape. There's a slight bluing on the very edges of the galaxy, possibly indicating the presence of younger stars or star forming regions. Overall the galaxy is smooth and appears relatively undisturbed with no clear signs of a major ongoing merger event.
