The galaxy presents as a relatively compact object. It has a bright, concentrated central region with a distinct, less luminous surrounding structure. The central region exhibits a white color, indicating a stellar population with a range of ages. Extending outwards from the core, a fainter and somewhat irregular halo is visible, exhibiting a slight cyan hue. This may suggest the presence of younger, hotter stars or ionized gas within this region. The overall morphology appears disturbed, possibly indicating a recent or ongoing interaction or merger. The object lacks any obvious spiral arms or well-defined disk structure. There is a hint of asymmetry. There are no clear tidal tails. The light is relatively diffuse.
