The galaxy presents as a single, moderately bright object with an apparent elongation. The light distribution suggests a relatively smooth morphology, potentially elliptical in shape. The core region exhibits a yellow-orange hue, possibly indicating an older stellar population and a lower rate of recent star formation in the central bulge. A distinct, bluer region appears as a secondary component, possibly a region of active star formation. There is a clear indication of a recent merger or interaction due to its disturbed morphology and offset core with different colors. The galaxy shows signs of on-going tidal interactions.
