The galaxy presents a somewhat elongated, disk-like appearance. It exhibits a relatively smooth overall structure, with a slightly brighter central region. Some faint structural details and disturbances are visible, particularly at the edges, which could indicate minor tidal interactions or recent merger activity. The color distribution appears fairly uniform, with a generally yellowish hue, though there are hints of bluer regions possibly indicating recent star formation. Based on these characteristics, it could potentially be a spiral galaxy undergoing transformation or a post-merger elliptical galaxy.
