The galaxy presents as an elongated structure, possibly indicating a late-stage merger or tidal interaction. The main body exhibits a smooth, relatively featureless morphology with a core of moderate luminosity. The central region displays a warm, yellowish hue, suggestive of an older stellar population and potentially significant dust extinction. 

There is an extended component to one side, appearing as a fainter, less defined region. This may represent a tidal tail or debris from an earlier interaction, or a second galaxy involved in a merger. This extended feature has a slight bluish tint in its outer edges, which may indicate some ongoing star formation activity. The overall color profile suggests a galaxy that has largely ceased forming new stars, but with some localized areas of more recent star formation. The galaxy's shape is notably non-circular, further supporting the hypothesis of a disturbed system.
