The galaxy appears to be a member of a pair, exhibiting a non-negligible degree of interaction with its companion. One galaxy presents a smoother morphology, suggesting an elliptical or lenticular classification. It displays a relatively spherical profile, though it appears slightly elongated. The dominant color is redder compared to the other galaxy. There may be evidence of a dust lane. The second galaxy appears bluer, indicating a younger stellar population and ongoing star formation. It shows a more irregular shape and a disturbed morphology, possibly indicative of tidal interactions. Overall, the system displays a mix of smooth and more actively star-forming characteristics, with signs of gravitational interaction influencing the appearance of both galaxies.
