The galaxy presents as a relatively smooth, centralized light distribution. There is a suggestion of a slight elongation, but it appears generally elliptical or spheroidal in shape. There's a bright central region that likely corresponds to the galactic nucleus. The light appears to fade gradually outward from the core, with no distinct spiral arms or bar structure visible in this image. There's some indication of faint, diffuse features around the galaxy suggesting a possible halo or extended stellar population. The overall color is dominated by a yellow-white hue, suggesting a higher abundance of older stellar populations. There may be a hint of bluer components, but they do not stand out. The slight color differences, combined with the apparent features, may indicate minor disturbances due to past interactions.
